texlive[46333] Master/texmf-dist: mandi (16jan18)
commits+karl at tug.org
commits+karl at tug.org
Tue Jan 16 23:45:03 CET 2018
Revision: 46333
http://tug.org/svn/texlive?view=revision&revision=46333
Author: karl
Date: 2018-01-16 23:45:03 +0100 (Tue, 16 Jan 2018)
Log Message:
-----------
mandi (16jan18)
Modified Paths:
--------------
trunk/Master/texmf-dist/doc/latex/mandi/mandi.pdf
trunk/Master/texmf-dist/doc/latex/mandi/vdemo.py
trunk/Master/texmf-dist/source/latex/mandi/mandi.dtx
trunk/Master/texmf-dist/source/latex/mandi/mandi.ins
trunk/Master/texmf-dist/tex/latex/mandi/mandi.sty
Modified: trunk/Master/texmf-dist/doc/latex/mandi/mandi.pdf
===================================================================
(Binary files differ)
Modified: trunk/Master/texmf-dist/doc/latex/mandi/vdemo.py
===================================================================
--- trunk/Master/texmf-dist/doc/latex/mandi/vdemo.py 2018-01-16 22:44:45 UTC (rev 46332)
+++ trunk/Master/texmf-dist/doc/latex/mandi/vdemo.py 2018-01-16 22:45:03 UTC (rev 46333)
@@ -1,5 +1,5 @@
-from __future__ import division, print_function
-from visual import *
+#
+from vpython import *
G = 6.7e-11
Modified: trunk/Master/texmf-dist/source/latex/mandi/mandi.dtx
===================================================================
--- trunk/Master/texmf-dist/source/latex/mandi/mandi.dtx 2018-01-16 22:44:45 UTC (rev 46332)
+++ trunk/Master/texmf-dist/source/latex/mandi/mandi.dtx 2018-01-16 22:45:03 UTC (rev 46333)
@@ -1,7 +1,7 @@
% \iffalse meta-comment
% !TEX TS-program = dtxmk
%
-% Copyright (C) 2016 by Paul J. Heafner <heafnerj at gmail.com>
+% Copyright (C) 2018 by Paul J. Heafner <heafnerj at gmail.com>
% ---------------------------------------------------------------------------
% This work may be distributed and/or modified under the conditions of the
% LaTeX Project Public License, either version 1.3 of this license or (at
@@ -32,13 +32,13 @@
%</internal>
%
%<*package>
-\ProvidesPackage{mandi}[2016/06/30 2.6.1 Macros for physics and astronomy]
+%%\ProvidesPackage{mandi}[2018/01/15 2.7.1 Macros for physics and astronomy]
\NeedsTeXFormat{LaTeX2e}[1999/12/01]
%</package>
%
%<*vdemo>
-from __future__ import division, print_function
-from visual import *
+#
+from vpython import *
G = 6.7e-11
@@ -71,6 +71,14 @@
\fi
%</internal>
%
+%<*internal>
+\ifx\fmtname\nameofplainTeX
+ \expandafter\endbatchfile
+\else
+ \expandafter\endgroup
+\fi
+%</internal>
+%
%<*driver>
\ProvidesFile{mandi.dtx}
%</driver>
@@ -84,7 +92,10 @@
\usepackage[left=0.75in,right=1.00in]{geometry} % main documentation
\usepackage{array,rotating,microtype} % accessory packages
\usepackage[listings,documentation]{tcolorbox} % workhorse package
+\usepackage{anyfontsize}
+\usepackage{float}
\usepackage{changepage} %%%%%%%%%%
+\usepackage{nameref}
\hypersetup{colorlinks, linktoc=all}
\tcbset{index german settings}
\tcbset{color hyperlink=blue}
@@ -92,6 +103,7 @@
\tcbset{color command=red}
\tcbset{doc head environment={interior style={fill,left color=red!15!white}}}
\tcbset{color environment=red}
+\tcbset{lefthand ratio=0.70}
\newcommandx{\ntodo}[2][1,usedefault]{%
\ifthenelse{\equal{#1}{}}
{\todo[size=\footnotesize,fancyline,caption={#2},color=yellow!40]
@@ -116,9 +128,9 @@
% \newcommand*{\mi}{\textit{Matter \& Interactions}}
% \hyphenation{Matter Interactions}
% \newcommand*{\opt}[1]{\textsf{\textbf{#1}}}
-% \newcommand*{\baseunits}{\textit{baseunits}}
-% \newcommand*{\drvdunits}{\textit{drvdunits}}
-% \newcommand*{\tradunits}{\textit{tradunits}}
+% \newcommand*{\baseunits}{\emph{baseunits}}
+% \newcommand*{\drvdunits}{\emph{drvdunits}}
+% \newcommand*{\tradunits}{\emph{tradunits}}
%
% \IndexPrologue{\section{Index}Page numbers refer to page where the
% corresponding entry is described. Not every command defined in the
@@ -125,7 +137,7 @@
% package is indexed. There may be commands similar to indexed commands
% described in relevant parts of the documentation.}
%
-% \CheckSum{6357}
+% \CheckSum{6548}
%
% \CharacterTable
% {Upper-case \A\B\C\D\E\F\G\H\I\J\K\L\M\N\O\P\Q\R\S\T\U\V\W\X\Y\Z
@@ -149,10 +161,17 @@
% \author{Paul J. Heafner
% (\href{mailto:heafnerj at gmail.com?subject=[Heafner]\%20mandi}
% {\nolinkurl{heafnerj at gmail.com}})}
-% \date{Version \fileversion~dated \filedate}
+% ^^A \date{Version \fileversion~dated \filedate}
+% \date{Version \mandiversion}
%
% \newgeometry{left=1.0in,right=1.0in,top=4.0in}
+% \pagenumbering{gobble}
+% \hypersetup{pageanchor=false}
+% \begin{titlepage}
% \maketitle
+% \end{titlepage}
+% \hypersetup{pageanchor=true}
+% \pagenumbering{arabic}
% \restoregeometry
%
% ^^A \centerline{\textbf{PLEASE DO NOT DISTRIBUTE THIS VERSION.}}
@@ -179,7 +198,7 @@
% type only what is necessary to get the desired result. What one types should
% correspond as closely as possible to what one thinks when writing. The package
% name derives from \mi
-% \footnote{See the \mi\ home page at \url{http://www.matterandinteractions.org/}
+% \footnote{See the \mi\ home page at \url{https://www.matterandinteractions.org/}
% for more information about this innovative introductory calculus-based physics
% curriculum.} by Ruth Chabay and Bruce Sherwood. The package certainly is rather
% tightly tied to that textbook but can be used for typesetting any document that
@@ -190,7 +209,7 @@
% There are other underlying philosophies and goals embedded within \mandi,
% all of which are summarized here. These philosophies are
% \begin{itemize}
-% \item to employ a \textit{type what you think} model for remembering commands
+% \item to employ a \emph{type what you think} model for remembering commands
% \item to relieve the user of having to explicitly worry about typesetting SI
% units
% \item to enforce certain concepts that are too frequently merged, such as the
@@ -198,7 +217,7 @@
% the same name for both)
% \item to enforce consistent terminology in the naming of quantities, with names
% that are both meaningful to introductory students and accurate
-% (e.g.\ \textit{duration} vs.\ \textit{time})
+% (e.g.\ \emph{duration} vs.\ \emph{time})
% \item to enforce consistent notation, especially for vector quantities
% \end{itemize}
%
@@ -210,8 +229,17 @@
% to build the documentation. I have not tested the build with with standard \LaTeX,
% which creates DVI files.
%
+% \changes{v2.7.0}{2018/01/11}{Added instructions for Overleaf users.}
+% \section{Overleaf Users}
+% \href{https://www.overleaf.com}{Overleaf} is an online \LaTeX\ environment with
+% widespread use. It uses a full \TeX/\LaTeX\ installation but doesn't always
+% have the latest version of every package installed. Sometimes packages are updated
+% more frequently than the large distributions are updated. If you want to always be
+% sure you're using the latest version of \mandi\ make sure the files
+% \pkgname{mandi.sty} and \pkgname{mandi.pdf} are in your Overleaf project folder.
+%
% \newpage
-% \section{Loading the Package}
+% \section{Loading the Package}\label{LoadingthePackage}
% To load \mandi\ with its default options, simply put the line |\usepackage{mandi}|
% in your document's preamble. To use the package's available options, put the line
% |\usepackage|\textbf{[}\opt{options}\textbf{]}|{mandi}| in your document's preamble.
@@ -227,6 +255,8 @@
% \changes{v2.6.0}{2016/05/18}{Option \opt{singleabsbars} renamed to
% \opt{singlemagbars}.}
% \changes{v2.6.0}{2016/05/23}{Loads the \pkgname{tensor} package for future use.}
+% \changes{v2.7.0}{2017/02/02}{Added blank output lines around mandi messages
+% during compilation.}
%
% \begin{itemize}
% \item \opt{boldvectors} gives bold letters for the kernels of vector names.
@@ -239,7 +269,7 @@
% \item \opt{singlemagbars} gives single bars in symbols for vector magnitudes.
% Double bars may be more familiar to students from their calculus courses.
% Double bars is the default.
-% \item \opt{approxconsts} gives \hypertarget{target4}{approximate} values of
+% \item \opt{approxconsts} gives \hypertarget{target1}{approximate} values of
% constants to one or two significant figures, depending on how they appear in
% \mi. Otherwise, the most precise currently available values are used. Precise
% constants is the default.
@@ -284,6 +314,10 @@
% \changes{v2.6.1}{2016/06/30}{Fixed \cs{mandiversion} so it displays correctly
% in math mode.}
%
+%\mandi\ loads the \pkgname{tensor} for likely future use. See that package's
+% documentation for its commands and how to use them. There are no known conflicts
+% between \mandi\ and \pkgname{tensor}.
+%
%\iffalse
%<*example>
%\fi
@@ -300,6 +334,8 @@
% \changes{v2.6.0}{2016/05/16}{Extensive revisions to documentation.}
% \changes{v2.6.0}{2016/05/02}{Created a student guide.}
% \changes{v2.6.1}{2016/06/30}{Fixed errors in Student Quick Guide documentation.}
+% \changes{v2.6.2}{2016/07/31}{Made minor changes to the documentation.}
+% \changes{v2.7.0}{2017/02/02}{Made numerous internal changes to eliminate warnings.}
% \newpage
% \section{Student Quick Guide}
% Use \refCom{vect} to put an arrow over a symbol to make it the symbol for a vector.
@@ -309,8 +345,8 @@
% gives \vectsub{p}{ball}.
%
% Use \refCom{magvect} or \refCom{magvectsub} to get the symbol for a vector's
-% magnitude. Typing |\magvect{p}| or |\magvectsub{p}{ball}| gives \magvect{p} or
-% \magvectsub{p}{ball}.
+% magnitude. Typing |\magvect{p}| gives \magvect{p}. Typing |\magvectsub{p}{ball}|
+% gives \magvectsub{p}{ball}.
%
% Use \refCom{dirvect} or \refCom{dirvectsub} to get the symbol for a vector's
% direction. Typing |\dirvect{p}| or |\dirvectsub{p}{ball}| gives \dirvect{p} or
@@ -355,6 +391,41 @@
% Use \refCom{define} to create a variable that can be used in an intermediate
% step in a solution. This is discussed later in this section.
%
+% To typeset a matrix in parentheses, use the \cs{pmatrix} environment by putting
+% the rows, between |\begin{pmatrix}| and |\end{pmatrix}|. Each row, except the
+% last, must end with |\\|. Within each row, separate the columns with |&|. Note
+% that \cs{pmatrix} typesets the matrix in parentheses. Use \cs{bmatrix} to typeset
+% it in square brackets and \cs{vmatrix} to typeset it in single vertical bars
+% to indicate a determinant. Use \cs{Vmatrix} to typeset it in double vertical
+% bars.
+%
+%\iffalse
+%<*example>
+%\fi
+ \begin{dispExample*}{sidebyside,colframe=white,colback=white, lefthand ratio=0.70}
+ A second rank tensor represented as a matrix.
+ \[\begin{pmatrix}
+ \hphantom{-}T_{00} & T_{01} & -T_{02} \\
+ -T_{10} & T_{11} & -T_{12} \\
+ \hphantom{-}T_{20} & T_{21} & \hphantom{-}T_{22}
+ \end{pmatrix}\]
+ Alternate notation for a matrix.
+ \[\begin{bmatrix}
+ \hphantom{-}T_{00} & T_{01} & -T_{02} \\
+ -T_{10} & T_{11} & -T_{12} \\
+ \hphantom{-}T_{20} & T_{21} & \hphantom{-}T_{22}
+ \end{bmatrix}\]
+ The determinant of a matrix.
+ \[\begin{vmatrix}
+ \hphantom{-}T_{00} & T_{01} & -T_{02} \\
+ -T_{10} & T_{11} & -T_{12} \\
+ \hphantom{-}T_{20} & T_{21} & \hphantom{-}T_{22}
+ \end{vmatrix}\]
+ \end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
% Encapsulate an entire problem solution in a \refEnv{problem} environment by
% putting it between |\begin{problem}| and |\end{problem}|.
%
@@ -364,9 +435,14 @@
% Use \cs{href} from the \pkgname{hyperref} package to link to URLs.
% |\href{http://glowscript.org}{GlowScript}| gives
% \href{http://glowscript.org}{GlowScript}. You can link to a specific
-% \href{http://goo.gl/wPMqjp}{GlowScript program} for this course. Links are
+% \href{http://goo.gl/wPMqjp}{GlowScript program} when necessary. Links are
% active.
%
+% Use \refCom{image} to insert diagrams. The diagram should be a PDF file. You
+% \emph{must} remember to specify a meaningful caption for the diagram. You must
+% also provide a unique label for the image so you can easily refer back to it
+% elsewhere in your document.
+%
% There are two main design goals behind this package. The first is to typeset
% numerical values of scalar and vector physical quantities and their SI units. The
% idea is to simply type a command corresponding to the quantity's name, specifying
@@ -382,7 +458,7 @@
%\iffalse
%<*example>
%\fi
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Efieldofparticle
\end{dispExample*}
%\iffalse
@@ -441,11 +517,11 @@
required arguments are, from left to right, a constant of proportionality, a
physical property of object 1, a physical property of object 2, the objects'
mutual separation, and a vector direction. In practice, these should all be
-provided in numerical form.
+provided in numerical form. Note that negative signs must be placed manually.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\genericinteractionplaces{}{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -458,11 +534,12 @@
Command for generic expression for an inverse square field. The four required
arguments are, from left to right, a constant of proportionality, a physical
property, relative distance to field point, and a vector direction. In practice,
-these should all be provided in numerical form.
+these should all be provided in numerical form. Note that negative signs must be
+placed manually.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\genericfieldofparticleplaces{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -475,11 +552,12 @@
Command for generic expression for an inverse square energy. The four required
arguments are, from left to right, a constant of proportionality, a physical
property of object 1, a physical property of object 2, and the objects' mutual
-separation. In practice, these should all be provided in numerical form.
+separation. In practice, these should all be provided in numerical form. Note that
+negative signs must be placed manually.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\genericpotentialenergyplaces{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -492,11 +570,11 @@
Command for gravitational interaction. The four required arguments are, from
left to right, the first object's mass, the second object's mass, the objects'
mutual separation, and a vector direction. In practice, these should all be
-provided in numerical form.
+provided in numerical form. Note that negative signs must be placed manually.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\gravitationalinteractionplaces{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -509,11 +587,11 @@
Command for gravitational field of a particle. The three required arguments are,
from left to right, the object's mass, the distance from the source to the field
point, and a vector direction. In practice, these should all be provided in
-numerical form.
+numerical form. Note that negative signs must be placed manually.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\gfieldofparticleplaces{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -526,11 +604,11 @@
Command for gravitational potential energy. The three required arguments are,
from left to right, the first object's mass, the second object's mass, and
the object's mutual distance. In practice, these should all be provided in
-numerical form.
+numerical form. Note the inclusion of the leading negative sign.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\gravitationalpotentialenergyplaces{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -542,11 +620,12 @@
{\marg{stiffness}\marg{stretch}\marg{direction}}
Command for a spring interaction. The three required arguments are, from left
to right, the spring stiffness, the spring's stretch, and a vector direction.
-In practice, these should all be provided in numerical form.
+In practice, these should all be provided in numerical form. Note that negative
+signs must be placed manually or absorbed into the displacement vector.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\springinteractionplaces{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -560,9 +639,9 @@
to right, the spring stiffness and the spring stretch. In practice, these should
be provided in numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\springpotentialenergyplaces{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -577,9 +656,9 @@
a dipole separation, the distance to the field point, and a vector direction. In
practice, these should all be provided in numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\genericelectricdipoleonaxisplaces{}{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -594,9 +673,9 @@
the distance to the field point, and a vector direction. In practice, these should
all be provided in numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\genericelectricdipoleplaces{}{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -611,9 +690,9 @@
separation, and a vector direction. In practice, these should all be provided in
numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\electricinteractionplaces{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -628,9 +707,9 @@
point, and a vector direction. In practice, these should all be provided in
numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\Efieldofparticleplaces{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -646,9 +725,9 @@
from the source to the field point. In practice, these should all be provided in
numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\Bfieldofparticleplaces{}{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -663,9 +742,9 @@
objects' mutual distance. In practice, these should all be provided in numerical
form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\electricpotentialenergyplaces{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -680,9 +759,9 @@
point, and a vector direction. In practice, these should all be provided in numerical
form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\electricdipoleonaxisplaces{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -696,14 +775,14 @@
to right, a charge, a dipole separation, the distance to the field point, and
a vector direction. In practice, these should all be provided in numerical form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\electricdipoleonbisectorplaces{}{}{}{}
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
%
-% The underlying strategy is to \textit{think about how you would say what you want
+% The underlying strategy is to \emph{think about how you would say what you want
% to write and then write it the way you would say it}. With a few exceptions, this
% is how \mandi\ works. You need not worry about units because \mandi\ knows what
% SI units go with which physical quantities. You can define new quantities so that
@@ -767,15 +846,16 @@
% \hyperlink{target2}{SI units} and the section on
% \hyperlink{target3}{physics quantities}.
%
+% \newpage
% \section{Features and Commands}
% \subsection{SI Base Units and Dimensions}
% This is not a tutorial on \hypertarget{target2}{SI units} and the user is assumed
% to be familiar with SI rules and usage. Begin by defining shortcuts for the units
% for the seven SI base quantities:
-% \textit{spatial displacement} (what others call \textit{length}), \textit{mass},
-% \textit{temporal displacement} (what others call \textit{time}, but we will call
-% it \textit{duration} in most cases), \textit{electric current}, \textit
-% {thermodynamic temperature}, \textit{amount}, and \textit{luminous intensity}.
+% \emph{spatial displacement} (what others call \emph{length}), \emph{mass},
+% \emph{temporal displacement} (what others call \emph{time}, but we will call
+% it \emph{duration} in most cases), \emph{electric current}, \emph
+% {thermodynamic temperature}, \emph{amount}, and \emph{luminous intensity}.
% These shortcuts are used internally and need not explicitly be invoked by the
% user.
%
@@ -783,7 +863,7 @@
%<*example>
%\fi
\begin{docCommand}{m}{}
- Command for \href{http://en.wikipedia.org/wiki/metre}{metre}, the SI unit of
+ Command for \href{https://en.wikipedia.org/wiki/metre}{metre}, the SI unit of
spatial displacement (length).
\end{docCommand}
%\iffalse
@@ -794,7 +874,7 @@
%<*example>
%\fi
\begin{docCommand}{kg}{}
- Command for \href{http://en.wikipedia.org/wiki/kilogram}{kilogram}, the SI unit
+ Command for \href{https://en.wikipedia.org/wiki/kilogram}{kilogram}, the SI unit
of mass.
\end{docCommand}
%\iffalse
@@ -805,7 +885,7 @@
%<*example>
%\fi
\begin{docCommand}{s}{}
- Command for \href{http://en.wikipedia.org/wiki/second}{second}, the SI unit
+ Command for \href{https://en.wikipedia.org/wiki/second}{second}, the SI unit
of temporal displacement (duration).
\end{docCommand}
%\iffalse
@@ -816,7 +896,7 @@
%<*example>
%\fi
\begin{docCommand}{A}{}
- Command for \href{http://en.wikipedia.org/wiki/ampere}{ampere}, the SI unit
+ Command for \href{https://en.wikipedia.org/wiki/ampere}{ampere}, the SI unit
of electric current.
\end{docCommand}
%\iffalse
@@ -827,7 +907,7 @@
%<*example>
%\fi
\begin{docCommand}{K}{}
- Command for \href{http://en.wikipedia.org/wiki/kelvin}{kelvin}, the SI unit
+ Command for \href{https://en.wikipedia.org/wiki/kelvin}{kelvin}, the SI unit
of thermodynamic temperature.
\end{docCommand}
%\iffalse
@@ -838,7 +918,7 @@
%<*example>
%\fi
\begin{docCommand}{mol}{}
- Command for \href{http://en.wikipedia.org/wiki/mole}{mole}, the SI unit of
+ Command for \href{https://en.wikipedia.org/wiki/mole}{mole}, the SI unit of
amount.
\end{docCommand}
%\iffalse
@@ -849,7 +929,7 @@
%<*example>
%\fi
\begin{docCommand}{cd}{}
- Command for \href{http://en.wikipedia.org/wiki/candela}{candela}, the SI
+ Command for \href{https://en.wikipedia.org/wiki/candela}{candela}, the SI
unit of luminous intensity.
\end{docCommand}
%\iffalse
@@ -862,7 +942,7 @@
% depending upon the application. Again, this is what we mean by \baseunits\ form.
%
% Certain combinations of the SI base units have nicknames and each such
-% combination and nickname constitutes a \textit{derived unit}. Derived units are
+% combination and nickname constitutes a \emph{derived unit}. Derived units are
% no more physically meaningful than the base units, they are merely nicknames for
% particular combinations of base units. An example of a derived unit is the
% newton, for which the symbol (it is not an abbreviation) is \newton. However,
@@ -869,8 +949,8 @@
% the symbol \newton\ is merely a nickname for a particular combination of base
% units. It is not the case that every unique combination of base units has a
% nickname, but those that do are usually named in honor of a scientist.
-% Incidentally, in such cases, the symbol is capitalized but the \textit{name}
-% of the unit is \textbf{never} capitalized. Thus we would write the name of the
+% Incidentally, in such cases, the symbol is capitalized but the \emph{name}
+% of the unit is \emph{never} capitalized. Thus we would write the name of the
% derived unit of force as newton and not Newton. Again, using these select
% nicknames for certain combinations of base units is what we mean by \drvdunits\
% form.
@@ -1161,11 +1241,38 @@
%\fi
%
% While we're at it, let's also go ahead and define a few non-SI units from
-% astronomy and astrophysics.
+% astronomy, astrophysics, and old school physics.
%
+%\changes{v2.6.3}{2016/09/08}{Added \cs{infeet}.}
+%\changes{v2.6.3}{2016/09/07}{Added \cs{infeetpersecond}.}
+%\changes{v2.6.3}{2016/09/08}{Added \cs{infeetpersecondsquared}.}
%\iffalse
%<*example>
%\fi
+\begin{docCommand}{infeet}{\marg{magnitude}}
+Command for magnitude of displacement in feet. This is still sometimes used
+in engineering applications and is frequently seen in older physics textbooks.
+\end{docCommand}
+\begin{docCommand}{infeetpersecond}{\marg{magnitude}}
+Command for magnitude of velocity in feet per second. This is still sometimes used
+in engineering applications and is frequently seen in older physics textbooks.
+\end{docCommand}
+\begin{docCommand}{infeetpersecondsquared}{\marg{magnitude}}
+Command for magnitude of acceleration in feet per second. This is still sometimes
+used in engineering applications and is frequently seen in older physics textbooks.
+\end{docCommand}
+\begin{dispExample*}{sidebyside}
+\infeet{5} \\
+\infeetpersecond{5} \\
+\infeetpersecondsquared{32}
+\end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
+%\iffalse
+%<*example>
+%\fi
\begin{docCommand}{planeangle}{\marg{magnitude}}
Command for plane angle in radians.
\end{docCommand}
@@ -2796,6 +2903,8 @@
%\chkquantity{temperature}
%\chkquantity{amount}
%\chkquantity{luminous}
+%\chkquantity{infeetpersecond}
+%\chkquantity{infeet}
%\chkquantity{planeangle}
%\chkquantity{solidangle}
%\chkquantity{velocity}
@@ -2868,12 +2977,29 @@
%\chkquantity{magneticcharge}
%\end{adjustwidth}
%
+% \subsection{When to Write Radians}\label{WhentoWriteRadians}
+% A word of clarification is in order for plane angles, solid angles, and other
+% angular quantities. There is the perpetually confusing issue of when to explicitly
+% write radians as a unit and when to omit it. The answer is that if the numerical
+% value of a quantity explicitly depends on the angular unit, then the unit should
+% be written. An example would be angular displacement; the numerical value obviously
+% depends on the unit used. If the numerical value of a quantity does not explicitly
+% depend on the angular unit, then the unit is omitted. An example would be the linear,
+% or translational, velocity or a particle in circular motion. This quantity doesn't
+% explicitly depends on the angular unit, so the angular unit is not written.
+%
+% Torque, angular impulse, and angular momentum present special a special problem
+% in that it is sometimes pedagogically helpful to explicitly include angular units
+% in their operational definitions. While this may not be in strict accordance
+% with SI standards, loading \mandi\ with the \opt{useradians} option includes
+% angular units in these quantities. See \nameref{LoadingthePackage} for details.
+%
% \newpage
%\changes{v2.5.0}{2015/10/09}{Documented precise and approximate
% constant values.}
% \subsection{Physical Constants}
% \subsubsection{Defining Physical Constants}
-% \mandi\ has many predefined \hypertarget{target1}{physical constants}.
+% \mandi\ has many predefined \hypertarget{target4}{physical constants}.
% This section explains how to use them.
%
%\iffalse
@@ -2894,7 +3020,7 @@
each part of the definition on a separate line.
\newphysicsconstant{planck}
{\ensuremath{h}}
- {\mi at p{6.6}{6.6261}\timestento{-34}}
+ {\mi at p{6.6}{6.626070040}\timestento{-34}}
{\m\squared\usk\kg\usk\reciprocal\s}
[\J\usk\s]
[\J\usk\s]
@@ -2934,7 +3060,10 @@
% \subsubsection{Predefined Physical Constants}
%
% In this section, precise values of constants are used. Approximate
-% values are available as an option when the package is loaded.
+% values are available as an option when the package is loaded. Precise values
+% are sourced as accurately as possible, beginning with Wikipedia and following
+% sources therein. I tried to use the most recent NIST or similarly authoritative
+% values. In no case did I make up any values.
%
%\iffalse
%<*example>
@@ -2942,9 +3071,9 @@
\begin{docCommand}{oofpez}{}
Coulomb constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\oofpezmathsymbol \approx \oofpez\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -2955,9 +3084,9 @@
\begin{docCommand}{oofpezcs}{}
Alternate form of Coulomb constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\oofpezcsmathsymbol \approx \oofpezcs\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -2981,9 +3110,9 @@
\begin{docCommand}{mzofp}{}
Biot-Savart constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\mzofpmathsymbol \approx \mzofp\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -2994,9 +3123,9 @@
\begin{docCommand}{vacuumpermeability}{}
Vacuum permeability.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\vacuumpermeabilitymathsymbol \approx \vacuumpermeability\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3007,9 +3136,9 @@
\begin{docCommand}{boltzmann}{}
Boltzmann constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\boltzmannmathsymbol \approx \boltzmann\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3020,9 +3149,9 @@
\begin{docCommand}{boltzmannineV}{}
Alternate form of Boltlzmann constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\boltzmannineVmathsymbol \approx \boltzmannineV\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3046,9 +3175,9 @@
\begin{docCommand}{planck}{}
Planck constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\planckmathsymbol \approx \planck\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3059,9 +3188,9 @@
\begin{docCommand}{planckineV}{}
Alternate form of Planck constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\planckmathsymbol \approx \planckineV\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3072,9 +3201,9 @@
\begin{docCommand}{planckbar}{}
Reduced Planck constant (Dirac constant).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\planckbarmathsymbol \approx \planckbar\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3085,9 +3214,9 @@
\begin{docCommand}{planckbarineV}{}
Alternate form of reduced Planck constant (Dirac constant).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\planckbarmathsymbol \approx \planckbarineV\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3098,9 +3227,9 @@
\begin{docCommand}{planckc}{}
Planck constant times light speed.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\planckcmathsymbol \approx \planckc\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3111,9 +3240,9 @@
\begin{docCommand}{planckcineV}{}
Alternate form of Planck constant times light speed.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\planckcineVmathsymbol \approx \planckcineV\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3124,9 +3253,9 @@
\begin{docCommand}{rydberg}{}
Rydberg constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\rydbergmathsymbol \approx \rydberg\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3137,9 +3266,9 @@
\begin{docCommand}{bohrradius}{}
Bohr radius.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\bohrradiusmathsymbol \approx \bohrradius\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3163,9 +3292,9 @@
\begin{docCommand}{avogadro}{}
Avogadro constant.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\avogadromathsymbol \approx \avogadro\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3202,9 +3331,9 @@
\begin{docCommand}{clight}{}
Magnitude of light's velocity (photon constant).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\clightmathsymbol \approx \clight\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3215,9 +3344,9 @@
\begin{docCommand}{clightinfeet}{}
Alternate of magnitude of light's velocity (photon constant).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\clightinfeetmathsymbol \approx \clightinfeet\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3228,9 +3357,9 @@
\begin{docCommand}{Ratom}{}
Approximate atomic radius.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Ratommathsymbol \approx \Ratom\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3241,9 +3370,9 @@
\begin{docCommand}{Mproton}{}
Proton mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Mprotonmathsymbol \approx \Mproton\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3254,9 +3383,9 @@
\begin{docCommand}{Mneutron}{}
Neutron mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Mneutronmathsymbol \approx \Mneutron\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3267,9 +3396,9 @@
\begin{docCommand}{Mhydrogen}{}
Hydrogen atom mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Mhydrogenmathsymbol \approx \Mhydrogen\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3280,9 +3409,9 @@
\begin{docCommand}{Melectron}{}
Electron mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Melectronmathsymbol \approx \Melectron\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3293,9 +3422,9 @@
\begin{docCommand}{echarge}{}
Elementary charge quantum.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\echargemathsymbol \approx \echarge\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3309,9 +3438,9 @@
\begin{docCommand}{qelectron}{}
Alias for \cs{Qelectron}.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Qelectronmathsymbol \approx \Qelectron\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3325,9 +3454,9 @@
\begin{docCommand}{qproton}{}
Alias for \cs{Qproton}.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\Qprotonmathsymbol \approx \Qproton\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3338,9 +3467,9 @@
\begin{docCommand}{MEarth}{}
Earth's mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\MEarthmathsymbol \approx \MEarth\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3351,9 +3480,9 @@
\begin{docCommand}{MMoon}{}
Moon's mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\MMoonmathsymbol \approx \MMoon\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3364,9 +3493,9 @@
\begin{docCommand}{MSun}{}
Sun's mass.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\MSunmathsymbol \approx \MSun\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3377,9 +3506,9 @@
\begin{docCommand}{REarth}{}
Earth's radius.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\REarthmathsymbol \approx \REarth\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3390,9 +3519,9 @@
\begin{docCommand}{RMoon}{}
Moon's radius.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\RMoonmathsymbol \approx \RMoon\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3403,9 +3532,9 @@
\begin{docCommand}{RSun}{}
Sun's radius.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\RSunmathsymbol \approx \RSun\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3419,9 +3548,9 @@
\begin{docCommand}{SEdist}{}
Alias for \refCom{ESdist}.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\ESdistmathsymbol \approx \SEdist\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3435,9 +3564,9 @@
\begin{docCommand}{MEdist}{}
Alias for \refCom{EMdist}.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\(\EMdistmathsymbol \approx \EMdist\)
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -3460,7 +3589,7 @@
%\fi
%
% Here are all the predefined constants and their units.
-%\begin{adjustwidth}{-0.5in}{-0.5in}
+%\begin{adjustwidth}{}{}
%
%\chkconstant{oofpez}
%\chkconstant{oofpezcs}
@@ -3851,12 +3980,26 @@
Symbol for direction of a vector quantity.
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\dirvect{p} or \direction{p}
+\dirvect{p}
\end{dispExample*}
%\iffalse
%</example>
%\fi
%
+%\changes{v2.7.0}{2017/04/13}{Added \cs{factorvect}.}
+%\iffalse
+%<*example>
+%\fi
+\begin{docCommand}{factorvect}{\marg{kernel}}
+Symbol for a vector factored into its magnitude and direction.
+\end{docCommand}
+\begin{dispExample*}{sidebyside}
+\factorvect{E}
+\end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
%\changes{v2.5.0}{2015/11/29}{Added \cs{componentalong}.}
%\iffalse
%<*example>
@@ -4375,11 +4518,8 @@
\begin{docCommand}{dirvectsub}{\marg{kernel}\marg{sub}}
Symbol for a subscripted vector's direction.
\end{docCommand}
-\begin{docCommand}{directionsub}{\marg{kernel}\marg{sub}}
-Alias for \refCom{dirvectsub}.
-\end{docCommand}
\begin{dispExample*}{sidebyside}
-\dirvectsub{p}{ball} or \directionsub{p}{ball}
+\dirvectsub{p}{ball}
\end{dispExample*}
%\iffalse
%</example>
@@ -4392,7 +4532,7 @@
Symbolic components of a subscripted vector.
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the vector \scompsvectsub{p}{ball}
+\scompsvectsub{p}{ball}
\end{dispExample*}
%\iffalse
%</example>
@@ -4405,7 +4545,7 @@
Isolates one component of a subscripted vector.
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the component \compvectsub{p}{ball}{z}
+\compvectsub{p}{ball}{z}
\end{dispExample*}
%\iffalse
%</example>
@@ -4419,7 +4559,7 @@
components.
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the magnitude \magvectsubscomps{p}{ball}
+\magvectsubscomps{p}{ball}
\end{dispExample*}
%\iffalse
%</example>
@@ -4435,8 +4575,8 @@
Identical to \refCom{dvectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the change \dvectsub{p}{ball} \\
-the change \Dvectsub{p}{ball}
+\dvectsub{p}{ball} \\
+\Dvectsub{p}{ball}
\end{dispExample*}
%\iffalse
%</example>
@@ -4452,8 +4592,8 @@
Identical to \refCom{scompsdvectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the vector \scompsdvectsub{p}{ball} \\
-the vector \scompsDvectsub{p}{ball}
+\scompsdvectsub{p}{ball} \\
+\scompsDvectsub{p}{ball}
\end{dispExample*}
%\iffalse
%</example>
@@ -4469,8 +4609,8 @@
Identical to \refCom{compdvectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the component \compdvectsub{p}{ball}{y} \\
-the component \compDvectsub{p}{ball}{y}
+\compdvectsub{p}{ball}{y} \\
+\compDvectsub{p}{ball}{y}
\end{dispExample*}
%\iffalse
%</example>
@@ -4487,8 +4627,8 @@
Identical to \refCom{dervectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the derivative \dervectsub{p}{ball}{t} \\
-the derivative \Dervectsub{p}{ball}{t}
+\dervectsub{p}{ball}{t} \\
+\Dervectsub{p}{ball}{t}
\end{dispExample*}
%\iffalse
%</example>
@@ -4505,8 +4645,8 @@
Identical to \refCom{dermagvectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the derivative \dermagvectsub{E}{ball}{t} \\
-the derivative \Dermagvectsub{E}{ball}{t}
+\dermagvectsub{E}{ball}{t} \\
+\Dermagvectsub{E}{ball}{t}
\end{dispExample*}
%\iffalse
%</example>
@@ -4523,8 +4663,8 @@
Identical to \refCom{scompsdervectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the vector \scompsdervectsub{p}{ball}{t} \\
-the vector \scompsDervectsub{p}{ball}{t}
+\scompsdervectsub{p}{ball}{t} \\
+\scompsDervectsub{p}{ball}{t}
\end{dispExample*}
%\iffalse
%</example>
@@ -4543,8 +4683,8 @@
Identical to \refCom{compdervectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the component \compdervectsub{p}{ball}{y}{t} \\
-the component \compDervectsub{p}{ball}{y}{t}
+\compdervectsub{p}{ball}{y}{t} \\
+\compDervectsub{p}{ball}{y}{t}
\end{dispExample*}
%\iffalse
%</example>
@@ -4561,8 +4701,8 @@
Identical to \refCom{magdervectsub} but uses \(\Delta\).
\end{docCommand}
\begin{dispExample*}{sidebyside}
-the derivative \magdervectsub{p}{ball}{t} \\
-the derivative \magDervectsub{p}{ball}{t}
+\magdervectsub{p}{ball}{t} \\
+\magDervectsub{p}{ball}{t}
\end{dispExample*}
%\iffalse
%</example>
@@ -4572,11 +4712,13 @@
% Now we get to commands that will save you many, many keystrokes. All of
% the naming conventions documented in earlier commands still apply. There
% are some new ones though. Every time you see |dot| you should think
-% \textit{dot product}. When you see |dots| you should think \textit{dot
+% \emph{dot product}. When you see |dots| you should think \emph{dot
% product in terms of symbolic components}. When you see |dote| you should
-% think \textit{dot product expanded as a sum}. These, along with the previous
+% think \emph{dot product expanded as a sum}. These, along with the previous
% naming conventions, handle many dot product expressions.
%
+%\changes{v2.7.0}{2.16/12/16}{Changed \cs{vectdotvect} to use \cs{cdot}.}
+%\changes{v2.7.0}{2016/12/16}{Added \cs{vectDotvect} to use \cs{bullet}.}
%\iffalse
%<*example>
%\fi
@@ -4583,8 +4725,12 @@
\begin{docCommand}{vectdotvect}{\marg{kernel1}\marg{kernel2}}
Symbol for dot of two vectors as a single symbol.
\end{docCommand}
+\begin{docCommand}{vectDotvect}{\marg{kernel1}\marg{kernel2}}
+Same as \cs{vectdotvect} but uses \cs{bullet}.
+\end{docCommand}
\begin{dispExample*}{sidebyside}
-\vectdotvect{\vect{F}}{\vect{v}}
+\vectdotvect{\vect{F}}{\vect{v}} \\
+\vectDotvect{\vect{F}}{\vect{v}}
\end{dispExample*}
%\iffalse
%</example>
@@ -4596,8 +4742,12 @@
\begin{docCommand}{vectdotsvect}{\marg{kernel1}\marg{kernel2}}
Symbol for dot of two vectors with symbolic components.
\end{docCommand}
+\begin{docCommand}{vectDotsvect}{\marg{kernel1}\marg{kernel2}}
+Same as \cs{vectdotsvect} but uses \cs{bullet}.
+\end{docCommand}
\begin{dispExample*}{sidebyside}
-\vectdotsvect{F}{v}
+\vectdotsvect{F}{v} \\
+\vectDotsvect{F}{v}
\end{dispExample*}
%\iffalse
%</example>
@@ -4657,7 +4807,7 @@
{\marg{kernel1}\marg{sub1}\marg{kernel2}\marg{sub2}}
Dot of two subscripted vectors with symbolic components.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\vectsubdotsvectsub{F}{grav}{r}{ball}
\end{dispExample*}
%\iffalse
@@ -4671,7 +4821,7 @@
{\marg{kernel1}\marg{sub1}\marg{kernel2}\marg{sub2}}
Dot of two subscripted vectors as an expanded sum.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\vectsubdotevectsub{F}{grav}{r}{ball}
\end{dispExample*}
%\iffalse
@@ -4690,7 +4840,7 @@
{\marg{kernel1}\marg{sub1}\marg{kernel2}\marg{sub2}}
Identical to \refCom{vectsubdotsdvectsub} but uses \(\Delta\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\vectsubdotsdvectsub{A}{ball}{B}{car} \\
\vectsubdotsDvectsub{A}{ball}{B}{car}
\end{dispExample*}
@@ -4710,7 +4860,7 @@
{\marg{kernel1}\marg{sub1}\marg{kernel2}\marg{sub2}}
Identical to \refCom{vectsubdotedvectsub} but uses \(\Delta\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\vectsubdotedvectsub{A}{ball}{B}{car} \\
\vectsubdoteDvectsub{A}{ball}{B}{car}
\end{dispExample*}
@@ -4728,7 +4878,7 @@
\begin{docCommand}{vectsubdotsDvect}{\marg{kernel1}\marg{sub1}\marg{kernel2}}
Identical to \refCom{vectsubdotsdvect} but uses \(\Delta\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\vectsubdotsdvect{A}{ball}{B} \\
\vectsubdotsDvect{A}{ball}{B}
\end{dispExample*}
@@ -4745,7 +4895,7 @@
\begin{docCommand}{vectsubdoteDvect}{\marg{kernel1}\marg{sub1}\marg{kernel2}}
Identical to \refCom{vectsubdotedvect} but uses \(\Delta\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\vectsubdotedvect{A}{ball}{B} \\
\vectsubdoteDvect{A}{ball}{B}
\end{dispExample*}
@@ -4831,7 +4981,7 @@
\begin{docCommand}{DervectdotsDvect}{\marg{kernel1}\marg{indvar}\marg{kernel2}}
Identical to \refCom{dervectdotsdvect} but uses \(\Delta\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\dervectdotsdvect{A}{t}{B} \\
\DervectdotsDvect{A}{t}{B}
\end{dispExample*}
@@ -5018,13 +5168,11 @@
\begin{docCommand}{efourfour}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\ezerozero, \ezeroone, \ezerotwo, \\
-\ezerothree, \ezerofour, \eoneone, \\
-\eonetwo, \eonethree, \eonefour, \\
-\etwoone, \etwotwo, \etwothree, \\
-\etwofour, \ethreeone, \ethreetwo, \\
-\ethreethree, \ethreefour, \efourone,\\
- \efourtwo, \efourthree, \efourfour
+\ezerozero, \ezeroone, \ezerotwo, \ezerothree, \ezerofour, \\
+\eoneone, \eonetwo, \eonethree, \eonefour, \etwoone, \\
+\etwotwo, \etwothree, \etwofour, \ethreeone, \ethreetwo, \\
+\ethreethree, \ethreefour, \efourone, \efourtwo, \efourthree, \\
+\efourfour
\end{dispExample*}
%\iffalse
%</example>
@@ -5120,13 +5268,11 @@
\begin{docCommand}{eufourfour}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\euzerozero, \euzeroone, \euzerotwo, \\
-\euzerothree, \euzerofour, \euoneone, \\
-\euonetwo, \euonethree, \euonefour, \\
-\eutwoone, \eutwotwo, \eutwothree, \\
-\eutwofour, \euthreeone, \euthreetwo, \\
-\euthreethree, \euthreefour, \eufourone, \\
-\eufourtwo, \eufourthree, \eufourfour
+\euzerozero, \euzeroone, \euzerotwo, \euzerothree, \euzerofour, \\
+\euoneone, \euonetwo, \euonethree, \euonefour, \eutwoone, \\
+\eutwotwo, \eutwothree, \eutwofour, \euthreeone, \euthreetwo, \\
+\euthreethree, \euthreefour, \eufourone, \eufourtwo, \eufourthree, \\
+\eufourfour
\end{dispExample*}
%\iffalse
%</example>
@@ -5208,13 +5354,11 @@
\begin{docCommand}{gfourfour}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\gzerozero, \gzeroone, \gzerotwo, \\
-\gzerothree, \gzerofour, \goneone, \\
-\gonetwo, \gonethree, \gonefour, \\
-\gtwoone, \gtwotwo, \gtwothree, \\
-\gtwofour, \gthreeone, \gthreetwo, \\
-\gthreethree, \gthreefour, \gfourone, \\
-\gfourtwo, \gfourthree, \gfourfour
+\gzerozero, \gzeroone, \gzerotwo, \gzerothree, \gzerofour, \\
+\goneone, \gonetwo, \gonethree, \gonefour, \gtwoone, \\
+\gtwotwo, \gtwothree, \gtwofour, \gthreeone, \gthreetwo, \\
+\gthreethree, \gthreefour, \gfourone, \gfourtwo, \gfourthree, \\
+\gfourfour
\end{dispExample*}
%\iffalse
%</example>
@@ -5268,13 +5412,11 @@
\begin{docCommand}{gufourfour}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\guzerozero, \guzeroone, \guzerotwo, \\
-\guzerothree, \guzerofour, \guoneone, \\
-\guonetwo, \guonethree, \guonefour, \\
-\gutwoone, \gutwotwo, \gutwothree, \\
-\gutwofour, \guthreeone, \guthreetwo, \\
-\guthreethree, \guthreefour, \gufourone, \\
-\gufourtwo, \gufourthree, \gufourfour
+\guzerozero, \guzeroone, \guzerotwo, \guzerothree, \guzerofour, \\
+\guoneone, \guonetwo, \guonethree, \guonefour, \gutwoone, \\
+\gutwotwo, \gutwothree, \gutwofour, \guthreeone, \guthreetwo, \\
+\guthreethree, \guthreefour, \gufourone, \gufourtwo, \gufourthree, \\
+\gufourfour
\end{dispExample*}
%\iffalse
%</example>
@@ -5447,9 +5589,8 @@
\begin{docCommand}{onetenth}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\(\onehalf, \onethird, \onefourth, \onefifth, \\
-\onesixth, \oneseventh, \oneeighth, \oneninth, \\
-\onetenth\)
+\(\onehalf, \onethird, \onefourth, \onefifth, \onesixth, \\
+\oneseventh, \oneeighth, \oneninth, \onetenth\)
\end{dispExample*}
%\iffalse
%</example>
@@ -5480,10 +5621,8 @@
\begin{docCommand}{twotenths}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\(\twooneths, \twohalves, \twothirds, \\
-\twofourths, \twofifths, \twosixths, \\
-\twosevenths, \twoeighths, \twoninths, \\
-\twotenths\)
+\(\twooneths, \twohalves, \twothirds, \twofourths, \twofifths, \\
+\twosixths, \twosevenths, \twoeighths, \twoninths, \twotenths\)
\end{dispExample*}
%\iffalse
%</example>
@@ -5514,10 +5653,8 @@
\begin{docCommand}{threetenths}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\(\threeoneths, \threehalves, \threethirds, \\
-\threefourths, \threefifths, \threesixths, \\
-\threesevenths, \threeeighths, \threeninths, \\
-\threetenths\)
+\(\threeoneths, \threehalves, \threethirds, \threefourths, \threefifths, \\
+\threesixths, \threesevenths, \threeeighths, \threeninths, \threetenths\)
\end{dispExample*}
%\iffalse
%</example>
@@ -5548,10 +5685,8 @@
\begin{docCommand}{fourtenths}{}
\end{docCommand}
\begin{dispExample*}{sidebyside}
-\(\fouroneths, \fourhalves, \fourthirds, \\
-\fourfourths, \fourfifths, \foursixths, \\
-\foursevenths, \foureighths, \fourninths, \\
-\fourtenths\)
+\(\fouroneths, \fourhalves, \fourthirds, \fourfourths, \fourfifths, \\
+\foursixths, \foursevenths, \foureighths, \fourninths, \fourtenths\)
\end{dispExample*}
%\iffalse
%</example>
@@ -5586,6 +5721,20 @@
%</example>
%\fi
%
+%\changes{v2.7.0}{2017/03/17}{Added \cs{dslashx} for inexact differentials.}
+%\iffalse
+%<*example>
+%\fi
+\begin{docCommand}{dslashx}{\marg{variable}}
+Symbol indicating an inexact differential. Frequently used in physics.
+\end{docCommand}
+\begin{dispExample*}{sidebyside}
+\( \dslashx{Q} \)
+\end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
%\changes{v2.6.0}{2016/05/10}{Replaced \cs{evalfromto} with \cs{evaluatedfromto}.}
%\iffalse
%<*example>
@@ -5963,9 +6112,9 @@
\begin{docCommand}{seriesexpx}{}
Series expansion of \(e^x\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\seriesexpx
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -5976,9 +6125,9 @@
\begin{docCommand}{seriessinx}{}
Series expansion of \(\sin x\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\seriessinx
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -5989,9 +6138,9 @@
\begin{docCommand}{seriescosx}{}
Series expansion of \(\cos x\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\seriescosx
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -6002,9 +6151,9 @@
\begin{docCommand}{seriestanx}{}
Series expansion of \(\tan x\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\seriestanx
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -6015,9 +6164,9 @@
\begin{docCommand}{seriesatox}{}
Series expansion of \(a^x\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\seriesatox
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -6028,9 +6177,9 @@
\begin{docCommand}{serieslnoneplusx}{}
Series expansion of \(\ln(1+x)\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\serieslnoneplusx
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -6041,9 +6190,9 @@
\begin{docCommand}{binomialseries}{}
Series expansion of \((1+x)^n\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample}
\binomialseries
-\end{dispExample*}
+\end{dispExample}
%\iffalse
%</example>
%\fi
@@ -6085,7 +6234,7 @@
\begin{docCommand}{Eulerlagrange}{\oarg{operand}}
Like \refCom{eulerlagrange} but uses \(\Delta\).
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\( \eulerlagrange \) or \( \eulerlagrange[x] \) \\
\( \Eulerlagrange \) or \( \Eulerlagrange[x] \)
\end{dispExample*}
@@ -6251,6 +6400,20 @@
%</example>
%\fi
%
+%\changes{v2.7.0}{2017/04/13}{Added \cs{circulation}.}
+%\iffalse
+%<*example>
+%\fi
+\begin{docCommand}{circulation}{\oarg{label}}
+Symbol for circulation of a vector field.
+\end{docCommand}
+\begin{dispExample*}{sidebyside}
+\circulation, \circulation[E]
+\end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
%\changes{v2.5.0}{2015/09/13}{Added \cs{inparens} for grouping with
% parentheses.}
%\changes{v2.6.0}{2016/05/02}{Changed placeholder to underscore.}
@@ -6342,7 +6505,7 @@
%<*example>
%\fi
\begin{docCommand}{Changein}{\marg{arg}}
-Notation for \textit{the change in a quantity}.
+Notation for \emph{the change in a quantity}.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\Changein{\vect{E}}
@@ -6756,7 +6919,7 @@
%<*example>
%\fi
\begin{docCommand}{isequals}{}
-Command for \textit{test-for-equality} operator.
+Command for \emph{test-for-equality} operator.
\end{docCommand}
\begin{dispExample*}{sidebyside}
5 \isequals 3
@@ -6811,7 +6974,7 @@
Same as \refCom{adjustedby} but puts parentheses around the operator.
\end{docCommand}
\begin{docCommand}{forevery}{}
-Operator the idea of for every.
+Operator for conveying the idea of for every.
\end{docCommand}
\begin{docCommand}{pforevery}{}
Same as \refCom{forevery} but puts parentheses around the operator.
@@ -6844,7 +7007,7 @@
%<*example>
%\fi
\begin{docCommand}{defines}{}
-Command for \textit{defines} or \textit{defined by} operator.
+Command for \emph{defines} or \emph{defined by} operator.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\vect{p} \defines \(\gamma m\)\vect{v}
@@ -6872,7 +7035,7 @@
%<*example>
%\fi
\begin{docCommand}{associates}{}
-Command for \textit{associated with} or \textit{associates with} operator
+Command for \emph{associated with} or \emph{associates with} operator
(for verbal concepts). This is conceptually different from the
\refCom{associated} or \refCom{passociated} operators.
\end{docCommand}
@@ -6887,7 +7050,7 @@
%<*example>
%\fi
\begin{docCommand}{becomes}{}
-Command for \textit{becomes} operator.
+Command for \emph{becomes} operator.
\end{docCommand}
\begin{dispExample*}{sidebyside}
\(\gamma m\)\vect{v} \becomes \(m\)\vect{v}
@@ -6951,7 +7114,7 @@
\begin{docCommand}{RHSmomentumprinciple}{}
Just the right hand side.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\momentumprinciple \\
\LHSmomentumprinciple \\
\RHSmomentumprinciple
@@ -6966,7 +7129,7 @@
\begin{docCommand}{momentumprinciplediff}{}
Expression for the momentum principle in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\momentumprinciplediff
\end{dispExample*}
%\iffalse
@@ -6986,8 +7149,8 @@
\begin{docCommand}{RHSenergyprinciple}{}
Just the right hand side.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
-\energyprinciple \\
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
+\energyprinciple \\
\LHSenergyprinciple \\
\RHSenergyprinciple
\end{dispExample*}
@@ -7001,7 +7164,7 @@
\begin{docCommand}{energyprinciplediff}{}
Expression for the energy principle in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\energyprinciplediff
\end{dispExample*}
%\iffalse
@@ -7020,7 +7183,7 @@
\begin{docCommand}{RHSangularmomentumprinciple}{}
Just the right hand side.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\angularmomentumprinciple \\
\LHSangularmomentumprinciple \\
\RHSangularmomentumprinciple
@@ -7035,7 +7198,7 @@
\begin{docCommand}{angularmomentumprinciplediff}{}
Expression for the angular momentum principle in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\angularmomentumprinciplediff
\end{dispExample*}
%\iffalse
@@ -7048,7 +7211,7 @@
\begin{docCommand}{gravitationalinteraction}{}
Expression for gravitational interaction.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\gravitationalinteraction
\end{dispExample*}
%\iffalse
@@ -7061,7 +7224,7 @@
\begin{docCommand}{electricinteraction}{}
Expression for electric interaction.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\electricinteraction
\end{dispExample*}
%\iffalse
@@ -7074,7 +7237,7 @@
\begin{docCommand}{springinteraction}{}
Expression for spring interaction.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\springinteraction
\end{dispExample*}
%\iffalse
@@ -7087,7 +7250,7 @@
\begin{docCommand}{gfieldofparticle}{}
Expression for a particle's gravitational field.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\gfieldofparticle
\end{dispExample*}
%\iffalse
@@ -7100,7 +7263,7 @@
\begin{docCommand}{Efieldofparticle}{}
Expression for a particle's electric field.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Efieldofparticle
\end{dispExample*}
%\iffalse
@@ -7113,7 +7276,7 @@
\begin{docCommand}{Bfieldofparticle}{}
Expression for a particle's magnetic field.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Bfieldofparticle
\end{dispExample*}
%\iffalse
@@ -7129,7 +7292,7 @@
\begin{docCommand}{Esys}{\oarg{label}}
Symbol for system energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Esys, \Esys[final], \Esys[initial]
\end{dispExample*}
%\iffalse
@@ -7142,7 +7305,7 @@
\begin{docCommand}{Us}{\oarg{label}}
Symbol for spring potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Us, \Us[final], \Us[initial]
\end{dispExample*}
%\iffalse
@@ -7155,7 +7318,7 @@
\begin{docCommand}{Ug}{\oarg{label}}
Symbol for gravitational potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Ug, \Ug[final], \Ug[initial]
\end{dispExample*}
%\iffalse
@@ -7168,7 +7331,7 @@
\begin{docCommand}{Ue}{\oarg{label}}
Symbol for electric potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Ue, \Ue[final], \Ue[initial]
\end{dispExample*}
%\iffalse
@@ -7181,7 +7344,7 @@
\begin{docCommand}{Ktrans}{\oarg{label}}
Symbol for translational kinetic energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Ktrans, \Ktrans[final], \Ktrans[initial]
\end{dispExample*}
%\iffalse
@@ -7194,7 +7357,7 @@
\begin{docCommand}{Krot}{\oarg{label}}
Symbol for rotational kinetic energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Krot, \Krot[final], \Krot[initial]
\end{dispExample*}
%\iffalse
@@ -7207,7 +7370,7 @@
\begin{docCommand}{Kvib}{\oarg{label}}
Symbol for vibrational kinetic energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Kvib, \Evib[final], \Evib[initial]
\end{dispExample*}
%\iffalse
@@ -7220,7 +7383,7 @@
\begin{docCommand}{Eparticle}{\oarg{label}}
Symbol for particle energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Eparticle, \Eparticle[final], \Eparticle[initial]
\end{dispExample*}
%\iffalse
@@ -7233,7 +7396,7 @@
\begin{docCommand}{Einternal}{\oarg{label}}
Symbol for internal energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Einternal, \Einternal[final], \Einternal[initial]
\end{dispExample*}
%\iffalse
@@ -7246,7 +7409,7 @@
\begin{docCommand}{Erest}{\oarg{label}}
Symbol for rest energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Erest, \Erest[final], \Erest[initial]
\end{dispExample*}
%\iffalse
@@ -7259,7 +7422,7 @@
\begin{docCommand}{Echem}{\oarg{label}}
Symbol for chemical energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Echem, \Echem[final], \Echem[initial]
\end{dispExample*}
%\iffalse
@@ -7272,7 +7435,7 @@
\begin{docCommand}{Etherm}{\oarg{label}}
Symbol for thermal energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Etherm, \Etherm[final], \Etherm[initial]
\end{dispExample*}
%\iffalse
@@ -7285,7 +7448,7 @@
\begin{docCommand}{Evib}{\oarg{label}}
Symbol for vibrational energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Evib, \Evib[final], \Evib[initial]
\end{dispExample*}
%\iffalse
@@ -7298,7 +7461,7 @@
\begin{docCommand}{Ephoton}{\oarg{label}}
Symbol for photon energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Ephoton, \Ephoton[final], \Ephoton[initial]
\end{dispExample*}
%\iffalse
@@ -7311,7 +7474,7 @@
\begin{docCommand}{DEsys}{}
Symbol for change in system energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEsys
\end{dispExample*}
%\iffalse
@@ -7324,7 +7487,7 @@
\begin{docCommand}{DUs}{}
Symbol for change in spring potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DUs
\end{dispExample*}
%\iffalse
@@ -7337,7 +7500,7 @@
\begin{docCommand}{DUg}{}
Symbol for change in gravitational potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DUg
\end{dispExample*}
%\iffalse
@@ -7350,7 +7513,7 @@
\begin{docCommand}{DUe}{}
Symbol for change in electric potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DUe
\end{dispExample*}
%\iffalse
@@ -7363,7 +7526,7 @@
\begin{docCommand}{DKtrans}{}
Symbol for change in translational kinetic energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DKtrans
\end{dispExample*}
%\iffalse
@@ -7376,7 +7539,7 @@
\begin{docCommand}{DKrot}{}
Symbol for change in rotational kinetic energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DKrot
\end{dispExample*}
%\iffalse
@@ -7389,7 +7552,7 @@
\begin{docCommand}{DKvib}{}
Symbol for change in vibrational kinetic energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DKvib
\end{dispExample*}
%\iffalse
@@ -7402,7 +7565,7 @@
\begin{docCommand}{DEparticle}{}
Symbol for change in particle energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEparticle
\end{dispExample*}
%\iffalse
@@ -7415,7 +7578,7 @@
\begin{docCommand}{DEinternal}{}
Symbol for change in internal energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEinternal
\end{dispExample*}
%\iffalse
@@ -7428,7 +7591,7 @@
\begin{docCommand}{DErest}{}
Symbol for change in rest energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DErest
\end{dispExample*}
%\iffalse
@@ -7441,7 +7604,7 @@
\begin{docCommand}{DEchem}{}
Symbol for change in chemical energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEchem
\end{dispExample*}
%\iffalse
@@ -7454,7 +7617,7 @@
\begin{docCommand}{DEtherm}{}
Symbol for change in thermal energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEtherm
\end{dispExample*}
%\iffalse
@@ -7467,7 +7630,7 @@
\begin{docCommand}{DEvib}{}
Symbol for change in vibrational energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEvib
\end{dispExample*}
%\iffalse
@@ -7480,7 +7643,7 @@
\begin{docCommand}{DEphoton}{}
Symbol for change in photon energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\DEphoton
\end{dispExample*}
%\iffalse
@@ -7493,7 +7656,7 @@
\begin{docCommand}{springpotentialenergy}{}
Expression for spring potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\springpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7506,7 +7669,7 @@
\begin{docCommand}{finalspringpotentnialenergy}{}
Expression for final spring potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\finalspringpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7519,7 +7682,7 @@
\begin{docCommand}{initialspringpotentialenergy}{}
Expression for initial spring potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\initialspringpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7532,7 +7695,7 @@
\begin{docCommand}{electricpotentialenergy}{}
Expression for electric potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\electricpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7545,7 +7708,7 @@
\begin{docCommand}{finalelectricpotentialenergy}{}
Expression for final electric potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\finalelectricpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7558,7 +7721,7 @@
\begin{docCommand}{initialelectricpotentialenergy}{}
Expression for initial electric potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\initialelectricpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7571,7 +7734,7 @@
\begin{docCommand}{gravitationalpotentialenergy}{}
Expression for gravitational potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\gravitationalpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7584,7 +7747,7 @@
\begin{docCommand}{finalgravitationalpotentialenergy}{}
Expression for final gravitational potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\finalgravitationalpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7597,7 +7760,7 @@
\begin{docCommand}{initialgravitationalpotentialenergy}{}
Expression for initial gravitational potential energy.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\initialgravitationalpotentialenergy
\end{dispExample*}
%\iffalse
@@ -7610,7 +7773,7 @@
\begin{docCommand}{ks}{}
Symbol for spring stiffness.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\ks
\end{dispExample*}
%\iffalse
@@ -7623,7 +7786,7 @@
\begin{docCommand}{Fnet}{}
Various symbols for net force.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Fnet, \Fnetext, \Fnetsys, \Fsub{ball,bat}
\end{dispExample*}
%\iffalse
@@ -7636,7 +7799,7 @@
\begin{docCommand}{Tnet}{}
Various symbols for net torque.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Tnet, \Tnetext, \Tnetsys, \Tsub{ball}
\end{dispExample*}
%\iffalse
@@ -7649,7 +7812,7 @@
\begin{docCommand}{Ltotal}{}
Various symbols for total angular momentum.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\Ltotal, \Lsys, \Lsub{ball}
\end{dispExample*}
%\iffalse
@@ -7665,7 +7828,7 @@
Left hand side of Maxwell's first equation in integral form. Note the
default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\LHSmaxwelliint \\
&\LHSmaxwelliint[S]
@@ -7681,7 +7844,7 @@
\begin{docCommand}{RHSmaxwelliint}{}
Right hand side of Maxwell's first equation in integral form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliint \]
\end{dispExample*}
%\iffalse
@@ -7695,7 +7858,7 @@
Alternate form of right hand side of Maxwell's first equation in
integral form. Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwelliinta \\
&\RHSmaxwelliinta[\upsilon]
@@ -7712,7 +7875,7 @@
Right hand side of Maxwell's first equation in integral form in
free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliintfree \]
\end{dispExample*}
%\iffalse
@@ -7726,7 +7889,7 @@
Maxwell's first equation in integral form.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliint \\
&\maxwelliint[S]
@@ -7743,7 +7906,7 @@
Alternate form of Maxwell's first equation in integral form.
Note the default values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliinta \\
&\maxwelliinta[S][\upsilon]
@@ -7760,7 +7923,7 @@
Maxwell's first equation in integral form in free space.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliintfree \\
&\maxwelliintfree[S]
@@ -7777,7 +7940,7 @@
Left hand side of Maxwell's second equation in integral form.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\LHSmaxwelliiint \\
&\LHSmaxwelliiint[S]
@@ -7793,7 +7956,7 @@
\begin{docCommand}{RHSmaxwelliiint}{}
Right hand side of Maxwell's second equation in integral form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliiint \]
\end{dispExample*}
%\iffalse
@@ -7807,7 +7970,7 @@
Right hand side of Maxwell's second equation in integral form
with magnetic monopoles.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliiintm \]
\end{dispExample*}
%\iffalse
@@ -7822,7 +7985,7 @@
integral form with magnetic monopoles. Note the default value of
the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwelliiintma \\
&\RHSmaxwelliiintma[\upsilon]
@@ -7839,7 +8002,7 @@
Right hand side of Maxwell's second equation in integral form in
free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliiintfree \]
\end{dispExample*}
%\iffalse
@@ -7853,7 +8016,7 @@
Maxwell's second equation in integral form. Note the default value
of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiint \\
&\maxwelliiint[S]
@@ -7870,7 +8033,7 @@
Maxwell's second equation in integral form with magnetic monopoles.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiintm \\
&\maxwelliiintm[S]
@@ -7887,7 +8050,7 @@
Alternate form of Maxwell's second equation in integral form with
magnetic monopoles. Note the default values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiintma \\
&\maxwelliiintma[S][\upsilon]
@@ -7904,7 +8067,7 @@
Maxwell's second equation in integral form in free space.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiintfree \\
&\maxwelliiintfree[S]
@@ -7921,7 +8084,7 @@
Left hand side of Maxwell's third equation in integral form.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\LHSmaxwelliiiint \\
&\LHSmaxwelliiiint[C]
@@ -7938,7 +8101,7 @@
Right hand side of Maxwell's third equation in integral form.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwelliiiint \\
&\RHSmaxwelliiiint[S]
@@ -7955,7 +8118,7 @@
Right hand side of Maxwell's third equation in integral form with
magnetic monopoles. Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwelliiiintm \\
&\RHSmaxwelliiiintm[S]
@@ -7973,7 +8136,7 @@
integral form with magnetic monopoles. Note the default value of
the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwelliiiintma \\
&\RHSmaxwelliiiintma[S]
@@ -7990,7 +8153,7 @@
Right hand side of Maxwell's third equation in integral form in
free space. Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwelliiiintfree \\
&\RHSmaxwelliiiintfree[S]
@@ -8007,7 +8170,7 @@
Maxwell's third equation in integral form. Note the default values of
the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiiint \\
&\maxwelliiiint[C][S]
@@ -8024,7 +8187,7 @@
Maxwell's third equation in integral form with magnetic monopoles.
Note the default values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiiintm \\
&\maxwelliiiintm[C][S]
@@ -8041,7 +8204,7 @@
Alternate form of Maxwell's third equation in integral form with magnetic
monopoles. Note the default values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiiintma \\
&\maxwelliiiintma[C][S]
@@ -8058,7 +8221,7 @@
Maxwell's third equation in integral form in free space. Note the default
values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwelliiiintfree \\
&\maxwelliiiintfree[C][S]
@@ -8075,7 +8238,7 @@
Left hand side of Maxwell's fourth equation in integral form.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\LHSmaxwellivint \\
&\LHSmaxwellivint[C]
@@ -8092,7 +8255,7 @@
Right hand side of Maxwell's fourth equation in integral form.
Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwellivint \\
&\RHSmaxwellivint[S]
@@ -8109,7 +8272,7 @@
Alternate form of right hand side of Maxwell's fourth equation in
integral form. Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwellivinta \\
&\RHSmaxwellivinta[S]
@@ -8126,7 +8289,7 @@
Right hand side of Maxwell's fourth equation in integral form in
free space. Note the default value of the optional argument.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\RHSmaxwellivintfree \\
&\RHSmaxwellivintfree[S]
@@ -8143,7 +8306,7 @@
Maxwell's fourth equation in integral form. Note the default values of
the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwellivint \\
&\maxwellivint[C][S]
@@ -8160,7 +8323,7 @@
Alternate form of Maxwell's fourth equation in integral form.
Note the default values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwellivinta \\
&\maxwellivinta[C][S]
@@ -8177,7 +8340,7 @@
Maxwell's fourth equation in integral form in free space.
Note the default values of the optional arguments.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{mysolution*}
&\maxwellivintfree \\
&\maxwellivintfree[C][S]
@@ -8193,7 +8356,7 @@
\begin{docCommand}{LHSmaxwellidif}{}
Left hand side of Maxwell's first equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \LHSmaxwellidif \]
\end{dispExample*}
%\iffalse
@@ -8206,7 +8369,7 @@
\begin{docCommand}{RHSmaxwellidif}{}
Right hand side of Maxwell's first equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwellidif \]
\end{dispExample*}
%\iffalse
@@ -8220,7 +8383,7 @@
Right hand side of Maxwell's first equation in differential form
in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwellidiffree \]
\end{dispExample*}
%\iffalse
@@ -8233,7 +8396,7 @@
\begin{docCommand}{maxwellidif}{}
Maxwell's first equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwellidif \]
\end{dispExample*}
%\iffalse
@@ -8246,7 +8409,7 @@
\begin{docCommand}{maxwellidiffree}{}
Maxwell's first equation in differential form in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwellidiffree \]
\end{dispExample*}
%\iffalse
@@ -8259,7 +8422,7 @@
\begin{docCommand}{LHSmaxwelliidif}{}
Left hand side of Maxwell's second equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \LHSmaxwelliidif \]
\end{dispExample*}
%\iffalse
@@ -8272,7 +8435,7 @@
\begin{docCommand}{RHSmaxwelliidif}{}
Right hand side of Maxwell's second equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliidif \]
\end{dispExample*}
%\iffalse
@@ -8286,7 +8449,7 @@
Right hand side of Maxwell's second equation in differential
form with magnetic monopoles.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliidifm \]
\end{dispExample*}
%\iffalse
@@ -8300,7 +8463,7 @@
Right hand side of Maxwell's second equation in differential
form in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliidiffree \]
\end{dispExample*}
%\iffalse
@@ -8313,7 +8476,7 @@
\begin{docCommand}{maxwelliidif}{}
Maxwell's second equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwelliidif \]
\end{dispExample*}
%\iffalse
@@ -8327,7 +8490,7 @@
Maxwell's second equation in differential form with magnetic
monopoles.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwelliidifm \]
\end{dispExample*}
%\iffalse
@@ -8340,7 +8503,7 @@
\begin{docCommand}{maxwellidiiffree}{}
Maxwell's second equation in differential form in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwelliidiffree \]
\end{dispExample*}
%\iffalse
@@ -8353,7 +8516,7 @@
\begin{docCommand}{LHSmaxwelliiidif}{}
Left hand side of Maxwell's third equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \LHSmaxwelliiidif \]
\end{dispExample*}
%\iffalse
@@ -8366,7 +8529,7 @@
\begin{docCommand}{RHSmaxwelliiidif}{}
Right hand side of Maxwell's third equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliiidif \]
\end{dispExample*}
%\iffalse
@@ -8380,7 +8543,7 @@
Right hand side of Maxwell's third equation in differential form
with magnetic monopoles.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliiidifm \]
\end{dispExample*}
%\iffalse
@@ -8394,7 +8557,7 @@
Right hand side of Maxwell's third equation in differential form
in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwelliiidiffree \]
\end{dispExample*}
%\iffalse
@@ -8407,7 +8570,7 @@
\begin{docCommand}{maxwelliiidif}{}
Maxwell's third equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwelliiidif \]
\end{dispExample*}
%\iffalse
@@ -8421,7 +8584,7 @@
Maxwell's third equation in differential form with magnetic
monopoles.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwelliiidifm \]
\end{dispExample*}
%\iffalse
@@ -8434,7 +8597,7 @@
\begin{docCommand}{maxwelliiidiffree}{}
Maxwell's third equation in differential form in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwelliiidiffree \]
\end{dispExample*}
%\iffalse
@@ -8447,7 +8610,7 @@
\begin{docCommand}{LHSmaxwellivdif}{}
Left hand side of Maxwell's fourth equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \LHSmaxwellivdif \]
\end{dispExample*}
%\iffalse
@@ -8460,7 +8623,7 @@
\begin{docCommand}{RHSmaxwellivdif}{}
Right hand side of Maxwell's fourth equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwellivdif \]
\end{dispExample*}
%\iffalse
@@ -8474,7 +8637,7 @@
Right hand side of Maxwell's fourth equation in differential form
in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSmaxwellivdiffree \]
\end{dispExample*}
%\iffalse
@@ -8487,7 +8650,7 @@
\begin{docCommand}{maxwellivdif}{}
Maxwell's fourth equation in differential form.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwellivdif \]
\end{dispExample*}
%\iffalse
@@ -8500,7 +8663,7 @@
\begin{docCommand}{maxwellivdiffree}{}
Maxwell's fourth equation in differential form in free space.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \maxwellivdiffree \]
\end{dispExample*}
%\iffalse
@@ -8515,7 +8678,7 @@
\begin{docCommand}{RHSlorentzforce}{}
Right hand side of Lorentz force.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSlorentzforce \]
\end{dispExample*}
%\iffalse
@@ -8528,7 +8691,7 @@
\begin{docCommand}{RHSlorentzforcem}{}
Right hand side of Lorentz force with magnetic monopoles.
\end{docCommand}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\[ \RHSlorentzforcem \]
\end{dispExample*}
%\iffalse
@@ -8537,16 +8700,20 @@
%
% \subsection{VPython and GlowScript Code}
% There are three ways to deal with VPython\footnote{See the VPython home page at
-% \url{http://vpython.org/} for more information.} and GlowScript\footnote{See the
-% GlowScript home page at \url{http://glowscript.org/} for more information.} code.
+% \url{https://vpython.org/} for more information.} and GlowScript\footnote{See the
+% GlowScript home page at \url{https://glowscript.org/} for more information.} code.
% With very few exceptions, VPython code and GlowScript code are identical. The
% commands with |vpython| in their names can handle both, but for semantic
% completeness there are corresponding commands with |glowscript| in their names.
+% Because Classic VPython will no longer be developed, the first line of all
+% VPython programs not used in GlowScript will conform to Jupyter syntax.
%
%\changes{v2.4.0}{2014/12/16}{\cs{vpythonline} now uses a uniform style.}
%\changes{v2.4.1}{2015/01/23}{Added more VPython keywords.}
%\changes{v2.5.0}{2016/01/26}{Added explicit mention of VPython and GlowScript.}
%\changes{v2.5.0}{2016/01/26}{Added GlowScript keywords.}
+%\changes{v2.7.0}{2017/02/02}{Changed first line of VPython programs to match
+% Jupyter syntax.}
%\iffalse
%<*example>
%\fi
@@ -8554,7 +8721,7 @@
Command for a single line of VPython or GlowScript code used inline.
\end{docCommand}
\begin{dispExample}
-\vpythonline{from __future__ import division, print_function}
+\vpythonline{from vpython import *}
\end{dispExample}
%\iffalse
%</example>
@@ -8585,8 +8752,8 @@
\end{docEnvironment}
\begin{dispExample}
\begin{vpythonblock}[Example VPython Listing]
- from __future__ import division,print_function
- from visual import *
+ from vpython import *
+
sphere(pos=vector(1,2,3),color=color.green)
# create a named arrow
MyArrow=arrow(pos=earth.pos,axis=fscale*Fnet,color=color.green)
@@ -8606,7 +8773,7 @@
\end{docEnvironment}
\begin{dispExample}
\begin{glowscriptblock}[Example GlowScript Listing]
-GlowScript 2.1 VPython
+GlowScript 2.3 VPython
Aarr = arrow(pos=vector(0,0,0),axis=A,color=color.red)
label(pos=Aarr.axis,text='A')
@@ -8869,7 +9036,7 @@
\begin{docCommand}{smallanswerform}{\oarg{name}\oarg{prompt}}
Editable answer form with height 0.10 that of current \cs{textheight}
and width 0.90 that of current \cs{linewidth}. The first argument isn't
-really optional, and \textbf{must} be different for each form used.
+really optional, and \emph{must} be different for each form used.
Content can be typed in the box and saved with a PDF editor or viewer
that supports PDF forms.
\end{docCommand}
@@ -9030,6 +9197,9 @@
\begin{docEnvironment}{miderivation}{}
Environment for mathematical derivations based on the |align| environment.
See \refEnv{mysolution} for how to handle long lines in this environment.
+Note that using this environment resets the counter for equation numbering.
+If you want continuous numbering throughout your document, use the |align|
+environment.
\end{docEnvironment}
\begin{docEnvironment}{miderivation*}{}
Like \refEnv{miderivation} but suppresses line numbers.
@@ -9051,9 +9221,25 @@
%</example>
%\fi
%
+%\changes{v2.6.3}{2016/09/02}{Added \cs{mistandard} for standards.}
%\iffalse
%<*example>
%\fi
+\begin{docEnvironment}{mistandard}{}
+Environment for standards for standards-based grading.
+\end{docEnvironment}
+\begin{dispExample}
+\begin{mistandard}
+ I can create a standard which reflects deep student learning.
+\end{mistandard}
+\end{dispExample}
+%\iffalse
+%</example>
+%\fi
+%
+%\iffalse
+%<*example>
+%\fi
\begin{docEnvironment}{bwinstructornote}{}
Like \refEnv{miinstructornote} but in black and grey.
\end{docEnvironment}
@@ -9127,6 +9313,22 @@
%</example>
%\fi
%
+%\changes{v2.6.3}{2016/09/02}{Added \cs{bwstandard} for standards.}
+%\iffalse
+%<*example>
+%\fi
+\begin{docEnvironment}{bwstandard}{}
+Like \refEnv{mistandard} but in black and grey.
+\end{docEnvironment}
+\begin{dispExample}
+\begin{bwstandard}
+ I can create a standard which reflects deep student learning.
+\end{bwstandard}
+\end{dispExample}
+%\iffalse
+%</example>
+%\fi
+%
%\changes{v2.5.0}{2015/10/14}{\cs{mysolution} now prints line numbers.}
%\changes{v2.5.0}{2015/10/14}{Added \cs{mysolution*} to suppress line numbers.}
%\changes{v2.5.0}{2016/01/26}{Added example showing how to handle long
@@ -9179,7 +9381,7 @@
%<*example>
%\fi
\begin{docEnvironment}{problem}{\marg{problemname}}
-Creates a simple environment for \hypertarget{target1}{problem solutions}. This
+Creates a simple environment for \hypertarget{target5}{problem solutions}. This
environment is mainly for students. Each new problem starts on a new page in an
effort to force organization upon students. The environment also creates a new
|enumerate| environment called |parts| for which labels are alphabetic,
@@ -9187,7 +9389,7 @@
is renamed \cs{problempart} to, again, help with organization for newcomers to
\LaTeX. A typical example would be structured as follows.
\end{docEnvironment}
-\begin{dispExample*}{sidebyside}
+\begin{dispExample*}{sidebyside, lefthand ratio=0.50}
\begin{problem}{Chapter 2 Problem 1}
This problem has two parts.
\begin{parts}
@@ -9203,6 +9405,7 @@
%\fi
%
%\changes{v2.6.0}{2016/05/02}{Added \cs{reason}.}
+%\changes{v2.7.0}{2017/02/02}{Changed \cs{reason} to use minipage.}
%\iffalse
%<*example>
%\fi
@@ -9239,14 +9442,26 @@
%</example>
%\fi
%
+%\changes{v2.6.3}{2016/09/11}{Loads the \pkgname{float} package for \cs{image}.}
+%\changes{v2.6.3}{2016/09/08}{Added scaling options to \cs{image}.}
+%\changes{v2.6.3}{2016/09/08}{Tweaked \cs{image} to work in documentation.}
+%\changes{v2.7.0}{2017/02/02}{Added fourth argument to \cs{image} for a label.}
%\iffalse
%<*example>
%\fi
-\begin{docCommand}{image}{\marg{imagefilename}\marg{caption}}
-Centered figure displayed actual size with caption.
+\begin{docCommand}{image}{\oarg{scaleorsizes}\marg{imagefilename}\marg{caption}\marg{label}}
+Centered figure displayed actual size with caption. The optional argument can be
+a scale factor (with 1 being the original image size), explicit \texttt{width}
+and/or \texttt{height} parameters, or even an \texttt{angle} for rotating the
+image. Be sure to give each image a unique label. This allows you to refer back
+to the image subsequently just by using the label.
\end{docCommand}
\begin{dispListing}
-\image{satellite.pdf}{Photograph of satellite}
+ \image{sampleimage.pdf}{An image shown actual size.}{img-label1}
+ \image[scale=1.5]{sampleimage.pdf}{An image scaled by 1.5 times.}{img-label2}
+ \image[height=1cm,width=2cm]{sampleimage.pdf}{An image resized.}{img-label3}
+ \image[width=0.8\textwidth]{sampleimage.pdf}{An image 80 percent the text width.}{img-label4}
+ \image[angle=45]{sampleimage.pdf}{An image actual size, rotated.}{img-label5}
\end{dispListing}
%\iffalse
%</example>
@@ -9266,6 +9481,35 @@
%</example>
%\fi
%
+%\changes{v2.7.0}{2017/09/01}{Added better looking parallel symbol.}
+%\iffalse
+%<*example>
+%\fi
+\begin{docCommand}{parallelto}{\marg{thing}}
+A better looking parallel symbol whose height is the same as the perpendicular
+symbol's height.
+\end{docCommand}
+\begin{dispExample*}{sidebyside}
+\(\vect{A}_{\parallelto\vect{B}}\) and \(\vect{A}_{\perpendicularto\vect{B}}\)
+\end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
+%\changes{v2.7.0}{2017/09/01}{Added an alias for the perpendicular symbol.}
+%\iffalse
+%<*example>
+%\fi
+\begin{docCommand}{perpendicularto}{\marg{thing}}
+An alias for the perpendicular symbol.
+\end{docCommand}
+\begin{dispExample*}{sidebyside}
+\(\vect{A}_{\parallelto\vect{B}}\) and \(\vect{A}_{\perpendicularto\vect{B}}\)
+\end{dispExample*}
+%\iffalse
+%</example>
+%\fi
+%
%\changes{v2.5.0}{2015/10/08}{Added \cs{qed} symbol.}
%\iffalse
%<*example>
@@ -9301,6 +9545,7 @@
\RequirePackage{etoolbox}
\RequirePackage{filehook}
\RequirePackage{extarrows}
+\RequirePackage{float}
\RequirePackage[T1]{fontenc}
\RequirePackage{graphicx}
\RequirePackage{epstopdf}
@@ -9317,7 +9562,7 @@
\RequirePackage{xspace}
\RequirePackage{ifthen}
\RequirePackage{calligra}
-\RequirePackage{hyperref}
+\RequirePackage[hypertexnames=false]{hyperref}
\hypersetup{colorlinks=true,urlcolor=blue}
\DeclareMathAlphabet{\mathcalligra}{T1}{calligra}{m}{n}
\DeclareFontShape{T1}{calligra}{m}{n}{<->s*[2.2]callig15}{}
@@ -9336,10 +9581,10 @@
line,linecolor,mag,mag2,make_trail,material,norm,normal,objects,opacity,points,pos,%
print,print_function,proj,pyramid,radians,radius,rate,retain,ring,rotate,scene,%
shaftwidth,shape,sign,size,space,sphere,text,trail_object,trail_type,True,twist,up,%
- vector,visual,width,offset,yoffset,GlowScript,VPython,trail_color,trail_radius,%
- pps,clear,False,CoffeeScript,graph,gdisplay,canvas,pause,vec,clone,compound,%
- vertex,triangle,quad,attach_trail,attach_arrow,textures,bumpmaps,print_options,%
- get_library,read_local_file},%
+ vector,visual,width,offset,yoffset,GlowScript,VPython,vpython,trail_color,%
+ trail_radius,pps,clear,False,CoffeeScript,graph,gdisplay,canvas,pause,vec,clone,%
+ compound,vertex,triangle,quad,attach_trail,attach_arrow,textures,bumpmaps,%
+ print_options,get_library,read_local_file},%
captionpos=b,% % position caption
frame=shadowbox,% % shadowbox around listing
rulesepcolor=\color{vshadowcolor},% % shadow color
@@ -9382,11 +9627,12 @@
%
% \begin{macrocode}
\newcommand*{\mandiversion}{\ifmmode%
- 2.6.1\mbox{ dated }2016/06/30%
+ 2.7.1\mbox{ dated }2018/01/15%
\else%
- 2.6.1 dated 2016/06/30%
+ 2.7.1 dated 2018/01/15%
\fi
}%
+\typeout{ }
\typeout{mandi: You're using mandi version \mandiversion.}
% \end{macrocode}
%
@@ -9405,7 +9651,7 @@
% \begin{macrocode}
\newcommand*{\per}{\ensuremath{/}}
\newcommand*{\usk}{\ensuremath{\cdot}}
-\newcommand*{\unit}[2]{\ensuremath{{#1}\,{#2}}}
+\newcommand*{\unit}[2]{\ensuremath{{#1}\;{#2}}}
\newcommand*{\ampere}{\ensuremath{\mathrm{A}}}
\newcommand*{\arcminute}{\ensuremath{'}}
\newcommand*{\arcsecond}{\ensuremath{''}}
@@ -9548,6 +9794,7 @@
\ifthenelse{\boolean{@optuseradians}}
{\typeout{mandi: You'll get radians in ang mom, ang impulse, and torque.}}
{\typeout{mandi: You won't get radians in ang mom, ang impulse, and torque.}}
+\typeout{ }
% \end{macrocode}
%
% \noindent This is a utility command for picking constants.
@@ -9600,11 +9847,14 @@
\newcommand*{\dimtemperature}{\ensuremath{\mathrm{\Theta}}}
\newcommand*{\dimamount}{\ensuremath{\mathrm{N}}}
\newcommand*{\dimluminous}{\ensuremath{\mathrm{J}}}
-\newcommand*{\indegrees}[1]{\unit{#1}{\degree}}
-\newcommand*{\inFarenheit}[1]{\unit{#1}{\degree\mathrm{F}}}
-\newcommand*{\inCelsius}[1]{\unit{#1}{\degree\mathrm{C}}}
-\newcommand*{\inarcminutes}[1]{\unit{#1}{\arcminute}}
-\newcommand*{\inarcseconds}[1]{\unit{#1}{\arcsecond}}
+\newcommand*{\infeet}[1]{\unit{#1}{\mathrm{ft}}}
+\newcommand*{\infeetpersecond}[1]{\unit{#1}{\mathrm{ft}\per\s}}
+\newcommand*{\infeetpersecondsquared}[1]{\unit{#1}{\mathrm{ft}\per\s\squared}}
+\newcommand*{\indegrees}[1]{\unit{#1}{\mkern-\thickmuskip\degree}}
+\newcommand*{\inFarenheit}[1]{\unit{#1}{\mkern-\thickmuskip\degree\mathrm{F}}}
+\newcommand*{\inCelsius}[1]{\unit{#1}{\mkern-\thickmuskip\degree\mathrm{C}}}
+\newcommand*{\inarcminutes}[1]{\unit{#1}{\mkern-\thickmuskip\arcminute}}
+\newcommand*{\inarcseconds}[1]{\unit{#1}{\mkern-\thickmuskip\arcsecond}}
\newcommand*{\ineV}[1]{\unit{#1}{\electronvolt}}
\newcommand*{\ineVocs}[1]{\unit{#1}{\mathrm{eV}\per c^2}}
\newcommand*{\ineVoc}[1]{\unit{#1}{\mathrm{eV}\per c}}
@@ -9665,11 +9915,11 @@
\newphysicsquantity{planeangle}%
{\m\usk\reciprocal\m}%
[\rad]%
- []
+ [\rad]
\newphysicsquantity{solidangle}%
{\m\squared\usk\reciprocalsquare\m}%
[\sr]%
- []
+ [\sr]
\newphysicsquantity{velocity}%
{\m\usk\reciprocal\s}%
[\m\usk\reciprocal\s]%
@@ -10033,6 +10283,7 @@
{\newcommand*{\dirvect}[1]{\ensuremath{\widehat{#1}}}}}
\newcommand*{\direction}[1]{\ensuremath{\mivector{#1}}}
\newcommand*{\vectordirection}{\direction}
+\newcommand*{\factorvect}[1]{\magvect{#1}\dirvect{#1}}
\newcommand*{\componentalong}[2]{\ensuremath{\mathrm{comp}_{#1}{#2}}}
\newcommand*{\expcomponentalong}[2]{\ensuremath{\frac{\vectdotvect{#2}{#1}}
{\magof{#1}}}}
@@ -10132,7 +10383,6 @@
\ifthenelse{\boolean{@optromanvectors}}
{\newcommand*{\dirvectsub}[2]{\ensuremath{\ssub{\widehat{\mathrm{#1}}}{#2}}}}
{\newcommand*{\dirvectsub}[2]{\ensuremath{\ssub{\widehat{#1}}{#2}}}}
-\newcommand*{\directionsub}{\dirvectsub}
\newcommand*{\dvectsub}[2]{\ensuremath{\mathrm{d}\vectsub{#1}{#2}}}
\newcommand*{\Dvectsub}[2]{\ensuremath{\Delta\vectsub{#1}{#2}}}
\newcommand*{\compdvectsub}[3]{\ensuremath{\mathrm{d}\compvectsub{#1}{#2}{#3}}}
@@ -10164,14 +10414,18 @@
\compDervectsub{#1}{#2}{x}{#3},%
\compDervectsub{#1}{#2}{y}{#3},%
\compDervectsub{#1}{#2}{z}{#3}\rv}}
-\newcommand*{\vectdotvect}[2]{\ensuremath{{#1}\bullet{#2}}}
-\newcommand*{\vectdotsvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsvect{#2}}}
+\newcommand*{\vectdotvect}[2]{\ensuremath{{#1}\cdot{#2}}}
+\newcommand*{\vectDotvect}[2]{\ensuremath{{#1}\bullet{#2}}}
+\newcommand*{\vectdotsvect}[2]{\ensuremath{\scompsvect{#1}\cdot\scompsvect{#2}}}
+\newcommand*{\vectDotsvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsvect{#2}}}
\newcommand*{\vectdotevect}[2]{\ensuremath{%
\compvect{#1}{x}\compvect{#2}{x}+%
\compvect{#1}{y}\compvect{#2}{y}+%
\compvect{#1}{z}\compvect{#2}{z}}}
-\newcommand*{\vectdotsdvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsdvect{#2}}}
-\newcommand*{\vectdotsDvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsDvect{#2}}}
+\newcommand*{\vectdotsdvect}[2]{\ensuremath{\scompsvect{#1}\cdot\scompsdvect{#2}}}
+\newcommand*{\vectDotsdvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsdvect{#2}}}
+\newcommand*{\vectdotsDvect}[2]{\ensuremath{\scompsvect{#1}\cdot\scompsDvect{#2}}}
+\newcommand*{\vectDotsDvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsDvect{#2}}}
\newcommand*{\vectdotedvect}[2]{\ensuremath{%
\compvect{#1}{x}\compdvect{#2}{x}+%
\compvect{#1}{y}\compdvect{#2}{y}+%
@@ -10181,6 +10435,8 @@
\compvect{#1}{y}\compDvect{#2}{y}+%
\compvect{#1}{z}\compDvect{#2}{z}}}
\newcommand*{\vectsubdotsvectsub}[4]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsvectsub{#3}{#4}}}
+\newcommand*{\vectsubDotsvectsub}[4]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsvectsub{#3}{#4}}}
\newcommand*{\vectsubdotevectsub}[4]{\ensuremath{%
\compvectsub{#1}{#2}{x}\compvectsub{#3}{#4}{x}+%
@@ -10187,8 +10443,12 @@
\compvectsub{#1}{#2}{y}\compvectsub{#3}{#4}{y}+%
\compvectsub{#1}{#2}{z}\compvectsub{#3}{#4}{z}}}
\newcommand*{\vectsubdotsdvectsub}[4]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsdvectsub{#3}{#4}}}
+\newcommand*{\vectsubDotsdvectsub}[4]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsdvectsub{#3}{#4}}}
\newcommand*{\vectsubdotsDvectsub}[4]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsDvectsub{#3}{#4}}}
+\newcommand*{\vectsubDotsDvectsub}[4]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsDvectsub{#3}{#4}}}
\newcommand*{\vectsubdotedvectsub}[4]{\ensuremath{%
\compvectsub{#1}{#2}{x}\compdvectsub{#3}{#4}{x}+%
@@ -10199,8 +10459,12 @@
\compvectsub{#1}{#2}{y}\compDvectsub{#3}{#4}{y}+%
\compvectsub{#1}{#2}{z}\compDvectsub{#3}{#4}{z}}}
\newcommand*{\vectsubdotsdvect}[3]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsdvect{#3}}}
+\newcommand*{\vectsubDotsdvect}[3]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsdvect{#3}}}
\newcommand*{\vectsubdotsDvect}[3]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsDvect{#3}}}
+\newcommand*{\vectsubDotsDvect}[3]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsDvect{#3}}}
\newcommand*{\vectsubdotedvect}[3]{\ensuremath{%
\compvectsub{#1}{#2}{x}\compdvect{#3}{x}+%
@@ -10211,8 +10475,12 @@
\compvectsub{#1}{#2}{y}\compDvect{#3}{y}+%
\compvectsub{#1}{#2}{z}\compDvect{#3}{z}}}
\newcommand*{\dervectdotsvect}[3]{\ensuremath{%
+ \scompsdervect{#1}{#2}\cdot\scompsvect{#3}}}
+\newcommand*{\dervectDotsvect}[3]{\ensuremath{%
\scompsdervect{#1}{#2}\bullet\scompsvect{#3}}}
\newcommand*{\Dervectdotsvect}[3]{\ensuremath{%
+ \scompsDervect{#1}{#2}\cdot\scompsvect{#3}}}
+\newcommand*{\DervectDotsvect}[3]{\ensuremath{%
\scompsDervect{#1}{#2}\bullet\scompsvect{#3}}}
\newcommand*{\dervectdotevect}[3]{\ensuremath{%
\compdervect{#1}{x}{#2}\compvect{#3}{x}+%
@@ -10223,8 +10491,12 @@
\compDervect{#1}{y}{#2}\compvect{#3}{y}+%
\compDervect{#1}{z}{#2}\compvect{#3}{z}}}
\newcommand*{\vectdotsdervect}[3]{\ensuremath{%
+ \scompsvect{#1}\cdot\scompsdervect{#2}{#3}}}
+\newcommand*{\vectDotsdervect}[3]{\ensuremath{%
\scompsvect{#1}\bullet\scompsdervect{#2}{#3}}}
\newcommand*{\vectdotsDervect}[3]{\ensuremath{%
+ \scompsvect{#1}\cdot\scompsDervect{#2}{#3}}}
+\newcommand*{\vectDotsDervect}[3]{\ensuremath{%
\scompsvect{#1}\bullet\scompsDervect{#2}{#3}}}
\newcommand*{\vectdotedervect}[3]{\ensuremath{%
\compvect{#1}{x}\compdervect{#2}{x}{#3}+%
@@ -10235,8 +10507,12 @@
\compvect{#1}{y}\compDervect{#2}{y}{#3}+%
\compvect{#1}{z}\compDervect{#2}{z}{#3}}}
\newcommand*{\dervectdotsdvect}[3]{\ensuremath{%
+ \scompsdervect{#1}{#2}\cdot\scompsdvect{#3}}}
+\newcommand*{\dervectDotsdvect}[3]{\ensuremath{%
\scompsdervect{#1}{#2}\bullet\scompsdvect{#3}}}
\newcommand*{\DervectdotsDvect}[3]{\ensuremath{%
+ \scompsDervect{#1}{#2}\cdot\scompsDvect{#3}}}
+\newcommand*{\DervectDotsDvect}[3]{\ensuremath{%
\scompsDervect{#1}{#2}\bullet\scompsDvect{#3}}}
\newcommand*{\dervectdotedvect}[3]{\ensuremath{%
\compdervect{#1}{x}{#2}\compdvect{#3}{x}+%
@@ -10253,8 +10529,12 @@
\newcommand*{\rtriplecross}[3]{\ensuremath{{#1}\boldsymbol{\times}%
\inparens{{#2}\boldsymbol{\times}{#3}}}}
\newcommand*{\ltriplescalar}[3]{\ensuremath{%
+ {#1}\boldsymbol{\times}{#2}\cdot{#3}}}
+\newcommand*{\ltripleScalar}[3]{\ensuremath{%
{#1}\boldsymbol{\times}{#2}\bullet{#3}}}
\newcommand*{\rtriplescalar}[3]{\ensuremath{%
+ {#1}\cdot{#2}\boldsymbol{\times}{#3}}}
+\newcommand*{\rtripleScalar}[3]{\ensuremath{%
{#1}\bullet{#2}\boldsymbol{\times}{#3}}}
\newcommand*{\ezero}{\ensuremath{\boldsymbol{e}_0}}
\newcommand*{\eone}{\ensuremath{\boldsymbol{e}_1}}
@@ -10463,7 +10743,7 @@
\left\lvert{#2}\right\rangle}}
\newphysicsconstant{oofpez}%
{\ensuremath{\frac{1}{\phantom{_o}4\pi\epsilon_0}}}%
- {\mi at p{9}{8.9876}\timestento{9}}%
+ {\mi at p{9}{8.9875517873681764}\timestento{9}}%
{\m\cubed\usk\kg\usk\reciprocalquartic\s\usk\A\reciprocalsquared}%
[\m\per\farad]%
[\newton\usk\m\squared\per\coulomb\squared]
@@ -10475,7 +10755,7 @@
[\N\usk\s\squared\per\C\squared]
\newphysicsconstant{vacuumpermittivity}%
{\ensuremath{\epsilon_0}}%
- {\mi at p{9.0}{8.8542}\timestento{-12}}%
+ {\mi at p{9.0}{8.854187817}\timestento{-12}}%
{\m\reciprocalcubed\usk\reciprocal\kg\usk\s\quarted\usk\A\squared}%
[\F\per\m]%
[\C\squared\per\N\usk\m\squared]
@@ -10493,103 +10773,103 @@
[\T\usk\m\per\A]
\newphysicsconstant{boltzmann}%
{\ensuremath{k_B}}%
- {\mi at p{1.4}{1.3806}\timestento{-23}}%
+ {\mi at p{1.4}{1.38064852}\timestento{-23}}%
{\m\squared\usk\kg\usk\reciprocalsquare\s\usk\reciprocal\K}%
[\joule\per\K]%
[\J\per\K]
\newphysicsconstant{boltzmannineV}%
{\ensuremath{k_B}}%
- {\mi at p{8.6}{8.6173}\timestento{-5}}%
+ {\mi at p{8.6}{8.6173303}\timestento{-5}}%
{\eV\usk\reciprocal\K}%
[\eV\per\K]%
[\eV\per\K]
\newphysicsconstant{stefanboltzmann}%
{\ensuremath{\sigma}}%
- {\mi at p{5.7}{5.6704}\timestento{-8}}%
+ {\mi at p{5.7}{5.670367}\timestento{-8}}%
{\kg\usk\s\reciprocalcubed\usk\K\reciprocalquarted}%
[\W\per\m\squared\usk\K^4]%
[\W\per\m\squared\usk\K\quarted]
\newphysicsconstant{planck}%
{\ensuremath{h}}%
- {\mi at p{6.6}{6.6261}\timestento{-34}}%
+ {\mi at p{6.6}{6.626070040}\timestento{-34}}%
{\m\squared\usk\kg\usk\reciprocal\s}%
[\J\usk\s]%
[\J\usk\s]
\newphysicsconstant{planckineV}%
{\ensuremath{h}}%
- {\mi at p{4.1}{4.1357}\timestento{-15}}%
+ {\mi at p{4.1}{4.135667662}\timestento{-15}}%
{\eV\usk\s}%
[\eV\usk\s]%
[\eV\usk\s]
\newphysicsconstant{planckbar}%
{\ensuremath{\hslash}}%
- {\mi at p{1.1}{1.0546}\timestento{-34}}%
+ {\mi at p{1.1}{1.054571800}\timestento{-34}}%
{\m\squared\usk\kg\usk\reciprocal\s}%
[\J\usk\s]%
[\J\usk\s]
\newphysicsconstant{planckbarineV}%
{\ensuremath{\hslash}}%
- {\mi at p{6.6}{6.5821}\timestento{-16}}%
+ {\mi at p{6.6}{6.582119514}\timestento{-16}}%
{\eV\usk\s}%
[\eV\usk\s]%
[\eV\usk\s]
\newphysicsconstant{planckc}%
{\ensuremath{hc}}%
- {\mi at p{2.0}{1.9864}\timestento{-25}}%
+ {\mi at p{2.0}{1.98644568}\timestento{-25}}%
{\m\cubed\usk\kg\usk\reciprocalsquare\s}%
[\J\usk\m]%
[\J\usk\m]
\newphysicsconstant{planckcineV}%
{\ensuremath{hc}}%
- {\mi at p{2.0}{1.9864}\timestento{-25}}%
+ {\mi at p{1240}{1.23984193}\timestento{3}}%
{\eV\usk\text{n}\m}%
[\eV\usk\text{n}\m]%
[\eV\usk\text{n}\m]
\newphysicsconstant{rydberg}%
{\ensuremath{\msub{R}{\infty}}}%
- {\mi at p{1.1}{1.0974}\timestento{7}}%
+ {\mi at p{1.1}{1.0973731568508}\timestento{7}}%
{\reciprocal\m}%
[\reciprocal\m]%
[\reciprocal\m]
\newphysicsconstant{bohrradius}%
{\ensuremath{a_0}}%
- {\mi at p{5.3}{5.2918}\timestento{-11}}%
+ {\mi at p{5.3}{5.2917721067}\timestento{-11}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{finestructure}%
{\ensuremath{\alpha}}%
- {\mi at p{\frac{1}{137}}{7.2974\timestento{-3}}}%
+ {\mi at p{\frac{1}{137}}{7.2973525664\timestento{-3}}}%
{}%
[]%
[]
\newphysicsconstant{avogadro}%
{\ensuremath{N_A}}%
- {\mi at p{6.0}{6.0221}\timestento{23}}%
+ {\mi at p{6.0}{6.022140857}\timestento{23}}%
{\reciprocal\mol}%
[\reciprocal\mol]%
[\reciprocal\mol]
\newphysicsconstant{universalgrav}%
{\ensuremath{G}}%
- {\mi at p{6.7}{6.6738}\timestento{-11}}%
+ {\mi at p{6.7}{6.67408}\timestento{-11}}%
{\m\cubed\usk\reciprocal\kg\usk\s\reciprocalsquared}%
[\J\usk\m\per\kg\squared]%
[\N\usk\m\squared\per\kg\squared]
\newphysicsconstant{surfacegravfield}%
{\ensuremath{g}}%
- {\mi at p{9.8}{9.80}}%
+ {\mi at p{9.8}{9.807}}%
{\m\usk\s\reciprocalsquared}%
[\N\per\kg]%
[\N\per\kg]
\newphysicsconstant{clight}%
{\ensuremath{c}}%
- {\mi at p{3}{2.9979}\timestento{8}}%
+ {\mi at p{3}{2.99792458}\timestento{8}}%
{\m\usk\reciprocal\s}%
[\m\per\s]%
[\m\per\s]
\newphysicsconstant{clightinfeet}%
{\ensuremath{c}}%
- {\mi at p{1}{0.9836}}%
+ {\mi at p{1}{0.983571}}%
{\text{ft}\usk\reciprocal{\text{n}\s}}%
[\text{ft}\per\text{n}\s]%
[\text{ft}\per\mathrm{n}\s]
@@ -10601,31 +10881,31 @@
[\m]
\newphysicsconstant{Mproton}%
{\ensuremath{m_p}}%
- {\mi at p{1.7}{1.6726}\timestento{-27}}%
+ {\mi at p{1.7}{1.672621898}\timestento{-27}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{Mneutron}%
{\ensuremath{m_n}}%
- {\mi at p{1.7}{1.6749}\timestento{-27}}%
+ {\mi at p{1.7}{1.674927471}\timestento{-27}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{Mhydrogen}%
{\ensuremath{m_H}}%
- {\mi at p{1.7}{1.6737}\timestento{-27}}%
+ {\mi at p{1.7}{1.6737236}\timestento{-27}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{Melectron}%
{\ensuremath{m_e}}%
- {\mi at p{9.1}{9.1094}\timestento{-31}}%
+ {\mi at p{9.1}{9.10938356}\timestento{-31}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{echarge}%
{\ensuremath{e}}%
- {\mi at p{1.6}{1.6022}\timestento{-19}}%
+ {\mi at p{1.6}{1.6021766208}\timestento{-19}}%
{\A\usk\s}%
[\C]%
[\C]
@@ -10655,61 +10935,61 @@
[\C]
\newphysicsconstant{MEarth}%
{\ensuremath{M_{\text{Earth}}}}%
- {\mi at p{6.0}{5.9736}\timestento{24}}%
+ {\mi at p{6.0}{5.97237}\timestento{24}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{MMoon}%
{\ensuremath{M_{\text{Moon}}}}%
- {\mi at p{7.3}{7.3459}\timestento{22}}%
+ {\mi at p{7.3}{7.342}\timestento{22}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{MSun}%
{\ensuremath{M_{\text{Sun}}}}%
- {\mi at p{2.0}{1.9891}\timestento{30}}%
+ {\mi at p{2.0}{1.98855}\timestento{30}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{REarth}%
{\ensuremath{R_{\text{Earth}}}}%
- {\mi at p{6.4}{6.3675}\timestento{6}}%
+ {\mi at p{6.4}{6.371}\timestento{6}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{RMoon}%
{\ensuremath{R_{\text{Moon}}}}%
- {\mi at p{1.7}{1.7375}\timestento{6}}%
+ {\mi at p{1.7}{1.7371}\timestento{6}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{RSun}%
{\ensuremath{R_{\text{Sun}}}}%
- {\mi at p{7.0}{6.9634}\timestento{8}}%
+ {\mi at p{7.0}{6.957}\timestento{8}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{ESdist}%
{\magvectsub{r}{ES}}%
- {\mi at p{1.5}{1.4960}\timestento{11}}%
+ {\mi at p{1.5}{1.496}\timestento{11}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{SEdist}%
{\magvectsub{r}{SE}}%
- {\mi at p{1.5}{1.4960}\timestento{11}}%
+ {\mi at p{1.5}{1.496}\timestento{11}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{EMdist}%
{\magvectsub{r}{EM}}%
- {\mi at p{3.8}{3.8440}\timestento{8}}%
+ {\mi at p{3.8}{3.81550}\timestento{8}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{MEdist}%
{\magvectsub{r}{ME}}%
- {\mi at p{3.8}{3.8440}\timestento{8}}%
+ {\mi at p{3.8}{3.81550}\timestento{8}}%
{\m}%
[\m]%
[\m]
@@ -10818,6 +11098,7 @@
\newcommand*{\sumoverall}[1]{\ensuremath{\displaystyle
\sum_{\substack{\text{\tiny{all }}\text{\tiny{{#1}}}}}}}
\newcommand*{\dx}[1]{\ensuremath{\,\mathrm{d}{#1}}}
+\newcommand*{\dslashx}[1]{\ensuremath{\,\mathchar'26\mkern-12mu \mathrm{d}{#1}}}
\newcommandx{\evaluatedfromto}[2][2,usedefault]{\ensuremath{%
\Bigg.\Bigg\rvert_{#1}^{#2}}}
\newcommand*{\evaluatedat}{\evaluatedfromto}
@@ -10920,6 +11201,7 @@
\newcommand*{\scripty}[1]{\ensuremath{\mathcalligra{#1}}}
\newcommand*{\Lagr}{\ensuremath{\mathcal{L}}}
\newcommandx{\flux}[1][1]{\ensuremath{\ssub{\Phi}{#1}}}
+\newcommandx{\circulation}[1][1]{\ensuremath{\ssub{\Gamma}{#1}}}
\newcommand*{\absof}[1]{\ensuremath{%
\left\lvert{\ifblank{#1}{\:\_\:}{#1}}\right\rvert}}
\newcommand*{\inparens}[1]{\ensuremath{%
@@ -10948,12 +11230,12 @@
\newcommand*{\hms}[3]{\ensuremath{%
{#1}^{\hour}{#2}^{\mathrm{m}}{#3}^{\s}}}
\newcommand*{\clockreading}{\hms}
-\newcommand*{\latitude}[1]{\unit{#1}{\degree}}
-\newcommand*{\latitudeN}[1]{\unit{#1}{\degree\;\mathrm{N}}}
-\newcommand*{\latitudeS}[1]{\unit{#1}{\degree\;\mathrm{S}}}
-\newcommand*{\longitude}[1]{\unit{#1}{\degree}}
-\newcommand*{\longitudeE}[1]{\unit{#1}{\degree\;\mathrm{E}}}
-\newcommand*{\longitudeW}[1]{\unit{#1}{\degree\;\mathrm{W}}}
+\newcommand*{\latitude}[1]{\unit{#1}{\mkern-\thickmuskip\degree}}
+\newcommand*{\latitudeN}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{N}}}
+\newcommand*{\latitudeS}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{S}}}
+\newcommand*{\longitude}[1]{\unit{#1}{\mkern-\thickmuskip\degree}}
+\newcommand*{\longitudeE}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{E}}}
+\newcommand*{\longitudeW}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{W}}}
\newcommand*{\ssub}[2]{\ensuremath{#1_{\text{#2}}}}
\newcommand*{\ssup}[2]{\ensuremath{#1^{\text{#2}}}}
\newcommand*{\ssud}[3]{\ensuremath{#1^{\text{#2}}_{\text{#3}}}}
@@ -11054,8 +11336,8 @@
\mivector{\_ , \_ , \_}}{#4}}}\times{{\ifblank{#5}{\mivector{\_ , \_ , \_}}{#5}}}}}
\newcommand*{\springinteractionplaces}[3]{\ensuremath{\inparens{#1}
\inparens{#2}{{\ifblank{#3}{\mivector{\_ , \_ , \_}}{#3}}}}}
-\newcommand*{\gravitationalpotentialenergyplaces}[3]{%
- -\genericpotentialenergyplaces{\universalgrav}{#1}{#2}{#3}}
+\newcommand*{\gravitationalpotentialenergyplaces}[3]{\ensuremath{%
+ -\genericpotentialenergyplaces{\universalgrav}{#1}{#2}{#3}}}
\newcommand*{\electricpotentialenergyplaces}[3]{%
\genericpotentialenergyplaces{\oofpez}{#1}{#2}{#3}}
\newcommand*{\springpotentialenergyplaces}[2]{\ensuremath{%
@@ -11590,6 +11872,21 @@
\end{align*}
\end{mdframed}
}%
+\mdfdefinestyle{mistandardstyle}{%
+ hidealllines=false,skipbelow=\baselineskip,skipabove=\baselineskip,
+ leftmargin=40pt,rightmargin=40pt,linewidth=1,roundcorner=10,
+ nobreak=true,
+ frametitle={STANDARD},
+ frametitlebackgroundcolor=cyan!60,frametitlerule=true,frametitlerulewidth=1,
+ backgroundcolor=cyan!25,
+ linecolor=black,fontcolor=black,shadow=true}
+\NewEnviron{mistandard}{%
+ \begin{mdframed}[style=mistandardstyle]
+ \begin{adjactivityanswer}[cyan!25][cyan!25][black]
+ \BODY
+ \end{adjactivityanswer}
+ \end{mdframed}
+}%
\mdfdefinestyle{bwinstructornotestyle}{%
hidealllines=false,skipbelow=\baselineskip,skipabove=\baselineskip,
leftmargin=40pt,rightmargin=40pt,linewidth=1,roundcorner=10,
@@ -11644,6 +11941,21 @@
\end{align*}
\end{mdframed}
}%
+\mdfdefinestyle{bwstandardstyle}{%
+ hidealllines=false,skipbelow=\baselineskip,skipabove=\baselineskip,
+ leftmargin=40pt,rightmargin=40pt,linewidth=1,roundcorner=10,
+ nobreak=true,
+ frametitle={STANDARD},
+ frametitlebackgroundcolor=gray!50,frametitlerule=true,frametitlerulewidth=1,
+ backgroundcolor=gray!20,
+ linecolor=black,fontcolor=black,shadow=true}
+\NewEnviron{bwstandard}{%
+ \begin{mdframed}[style=bwstandardstyle]
+ \begin{adjactivityanswer}[gray!20][gray!20][black]
+ \BODY
+ \end{adjactivityanswer}
+ \end{mdframed}
+}%
\NewEnviron{mysolution}{%
\setcounter{equation}{0}
\begin{align}
@@ -11662,21 +11974,23 @@
\newlist{parts}{enumerate}{2}%
\setlist[parts]{label=(\alph*)}}{\newpage}
\newcommand{\problempart}{\item}%
-\newcommand{\reason}[1]{\parbox{2cm}{#1}}
+\newcommand{\reason}[1]{\begin{minipage}{5cm}{#1}\end{minipage}}
\newcommand*{\checkpoint}{%
\vspace{1cm}\begin{center}%
\colorbox{yellow!80}{|--------- CHECKPOINT ---------|}%
\end{center}}%
-\newcommand*{\image}[2]{%
- \begin{figure}[h!]
+\newcommandx*{\image}[4][1={scale=1},usedefault]{%
+ \begin{figure}[H]
\begin{center}%
- \includegraphics[scale=1]{#1}%
- \caption{#2}%
- \label{#1}%
+ \includegraphics[#1]{#2}%
\end{center}%
+ \caption{#3}%
+ \label{#4}%
\end{figure}}
-%\changes{v2.5.0}{2015/09/13}{Changed behavior of \cs{sneakyone}.}
\newcommand*{\sneakyone}[1]{\ensuremath{\cancelto{1}{#1}}}
+\newcommand*{\parallelto}{\ensuremath{{{\mkern3mu\vphantom{\perp}\vrule depth 0pt
+ \mkern2mu\vrule depth 0pt\mkern3mu}}}}
+\newcommand*{\perpendicularto}{\ensuremath{\perp}}
\newcommand*{\qed}{\ensuremath{\text{ Q.E.D.}}}
\newcommand*{\chkquantity}[1]{%
\begin{center}
@@ -11689,11 +12003,13 @@
}%
\newcommand*{\chkconstant}[1]{%
\begin{center}
- \begin{tabular}{C{4cm} C{2cm} C{3cm} C{3cm} C{3cm} C{3cm}}
- name & symbol & value & baseunit & drvdunit & tradunit \tabularnewline
- \cs{#1} & \csname #1mathsymbol\endcsname & \csname #1value\endcsname &
- \csname #1onlybaseunit\endcsname & \csname #1onlydrvdunit\endcsname &
- \csname #1onlytradunit\endcsname
+ \begin{tabular}{C{4cm} C{4cm} C{4cm}}
+ name & symbol & value \tabularnewline
+ \cs{#1} & \csname #1mathsymbol\endcsname & \csname #1value\endcsname
+ \tabularnewline
+ baseunit & drvdunit & tradunit \tabularnewline
+ \csname #1onlybaseunit\endcsname & \csname #1onlydrvdunit\endcsname &
+ \csname #1onlytradunit\endcsname
\end{tabular}
\end{center}
}%
@@ -11706,7 +12022,7 @@
% Special thanks also to Herbert Schulz for his custom \texttt{dtx} engine for
% \texttt{TeXShop}. Very special thanks to Ulrich Diez for providing the mechanism
% that defines physics quantities and constants. Also very special thanks to
-% student who helped test recent version of this package.
+% students who helped test recent versions of this package.
%
% \iffalse
%</package>
Modified: trunk/Master/texmf-dist/source/latex/mandi/mandi.ins
===================================================================
--- trunk/Master/texmf-dist/source/latex/mandi/mandi.ins 2018-01-16 22:44:45 UTC (rev 46332)
+++ trunk/Master/texmf-dist/source/latex/mandi/mandi.ins 2018-01-16 22:45:03 UTC (rev 46333)
@@ -6,7 +6,7 @@
%%
%% mandi.dtx (with options: `install')
%%
-%% Copyright (C) 2016 by Paul J. Heafner <heafnerj at gmail.com>
+%% Copyright (C) 2018 by Paul J. Heafner <heafnerj at gmail.com>
%% ---------------------------------------------------------------------------
%% This work may be distributed and/or modified under the conditions of the
%% LaTeX Project Public License, either version 1.3 of this license or (at
@@ -34,7 +34,7 @@
\usedir{tex/latex/mandi}
\preamble
-Copyright (C) 2016 by Paul J. Heafner <heafnerj at gmail.com>
+Copyright (C) 2018 by Paul J. Heafner <heafnerj at gmail.com>
---------------------------------------------------------------------------
This work may be distributed and/or modified under the conditions of the
LaTeX Project Public License, either version 1.3 of this license or (at
Modified: trunk/Master/texmf-dist/tex/latex/mandi/mandi.sty
===================================================================
--- trunk/Master/texmf-dist/tex/latex/mandi/mandi.sty 2018-01-16 22:44:45 UTC (rev 46332)
+++ trunk/Master/texmf-dist/tex/latex/mandi/mandi.sty 2018-01-16 22:45:03 UTC (rev 46333)
@@ -6,7 +6,7 @@
%%
%% mandi.dtx (with options: `package')
%%
-%% Copyright (C) 2016 by Paul J. Heafner <heafnerj at gmail.com>
+%% Copyright (C) 2018 by Paul J. Heafner <heafnerj at gmail.com>
%% ---------------------------------------------------------------------------
%% This work may be distributed and/or modified under the conditions of the
%% LaTeX Project Public License, either version 1.3 of this license or (at
@@ -28,7 +28,7 @@
%% vdemo.py.
%% ---------------------------------------------------------------------------
%%
-\ProvidesPackage{mandi}[2016/06/30 2.6.1 Macros for physics and astronomy]
+%%\ProvidesPackage{mandi}[2018/01/15 2.7.1 Macros for physics and astronomy]
\NeedsTeXFormat{LaTeX2e}[1999/12/01]
\RequirePackage{amsmath}
@@ -43,6 +43,7 @@
\RequirePackage{etoolbox}
\RequirePackage{filehook}
\RequirePackage{extarrows}
+\RequirePackage{float}
\RequirePackage[T1]{fontenc}
\RequirePackage{graphicx}
\RequirePackage{epstopdf}
@@ -59,7 +60,7 @@
\RequirePackage{xspace}
\RequirePackage{ifthen}
\RequirePackage{calligra}
-\RequirePackage{hyperref}
+\RequirePackage[hypertexnames=false]{hyperref}
\hypersetup{colorlinks=true,urlcolor=blue}
\DeclareMathAlphabet{\mathcalligra}{T1}{calligra}{m}{n}
\DeclareFontShape{T1}{calligra}{m}{n}{<->s*[2.2]callig15}{}
@@ -78,10 +79,10 @@
line,linecolor,mag,mag2,make_trail,material,norm,normal,objects,opacity,points,pos,%
print,print_function,proj,pyramid,radians,radius,rate,retain,ring,rotate,scene,%
shaftwidth,shape,sign,size,space,sphere,text,trail_object,trail_type,True,twist,up,%
- vector,visual,width,offset,yoffset,GlowScript,VPython,trail_color,trail_radius,%
- pps,clear,False,CoffeeScript,graph,gdisplay,canvas,pause,vec,clone,compound,%
- vertex,triangle,quad,attach_trail,attach_arrow,textures,bumpmaps,print_options,%
- get_library,read_local_file},%
+ vector,visual,width,offset,yoffset,GlowScript,VPython,vpython,trail_color,%
+ trail_radius,pps,clear,False,CoffeeScript,graph,gdisplay,canvas,pause,vec,clone,%
+ compound,vertex,triangle,quad,attach_trail,attach_arrow,textures,bumpmaps,%
+ print_options,get_library,read_local_file},%
captionpos=b,% % position caption
frame=shadowbox,% % shadowbox around listing
rulesepcolor=\color{vshadowcolor},% % shadow color
@@ -121,11 +122,12 @@
\DeclareOption{useradians}{\setboolean{@optuseradians}{true}}
\ProcessOptions\relax
\newcommand*{\mandiversion}{\ifmmode%
- 2.6.1\mbox{ dated }2016/06/30%
+ 2.7.1\mbox{ dated }2018/01/15%
\else%
- 2.6.1 dated 2016/06/30%
+ 2.7.1 dated 2018/01/15%
\fi
}%
+\typeout{ }
\typeout{mandi: You're using mandi version \mandiversion.}
\@ifpackageloaded{amssymb}{%
\csundef{square}
@@ -136,7 +138,7 @@
}%
\newcommand*{\per}{\ensuremath{/}}
\newcommand*{\usk}{\ensuremath{\cdot}}
-\newcommand*{\unit}[2]{\ensuremath{{#1}\,{#2}}}
+\newcommand*{\unit}[2]{\ensuremath{{#1}\;{#2}}}
\newcommand*{\ampere}{\ensuremath{\mathrm{A}}}
\newcommand*{\arcminute}{\ensuremath{'}}
\newcommand*{\arcsecond}{\ensuremath{''}}
@@ -267,6 +269,7 @@
\ifthenelse{\boolean{@optuseradians}}
{\typeout{mandi: You'll get radians in ang mom, ang impulse, and torque.}}
{\typeout{mandi: You won't get radians in ang mom, ang impulse, and torque.}}
+\typeout{ }
\ifthenelse{\boolean{@optapproxconsts}}
{\newcommand*{\mi at p}[2]{#1}} % approximate value
{\newcommand*{\mi at p}[2]{#2}} % precise value
@@ -284,11 +287,14 @@
\newcommand*{\dimtemperature}{\ensuremath{\mathrm{\Theta}}}
\newcommand*{\dimamount}{\ensuremath{\mathrm{N}}}
\newcommand*{\dimluminous}{\ensuremath{\mathrm{J}}}
-\newcommand*{\indegrees}[1]{\unit{#1}{\degree}}
-\newcommand*{\inFarenheit}[1]{\unit{#1}{\degree\mathrm{F}}}
-\newcommand*{\inCelsius}[1]{\unit{#1}{\degree\mathrm{C}}}
-\newcommand*{\inarcminutes}[1]{\unit{#1}{\arcminute}}
-\newcommand*{\inarcseconds}[1]{\unit{#1}{\arcsecond}}
+\newcommand*{\infeet}[1]{\unit{#1}{\mathrm{ft}}}
+\newcommand*{\infeetpersecond}[1]{\unit{#1}{\mathrm{ft}\per\s}}
+\newcommand*{\infeetpersecondsquared}[1]{\unit{#1}{\mathrm{ft}\per\s\squared}}
+\newcommand*{\indegrees}[1]{\unit{#1}{\mkern-\thickmuskip\degree}}
+\newcommand*{\inFarenheit}[1]{\unit{#1}{\mkern-\thickmuskip\degree\mathrm{F}}}
+\newcommand*{\inCelsius}[1]{\unit{#1}{\mkern-\thickmuskip\degree\mathrm{C}}}
+\newcommand*{\inarcminutes}[1]{\unit{#1}{\mkern-\thickmuskip\arcminute}}
+\newcommand*{\inarcseconds}[1]{\unit{#1}{\mkern-\thickmuskip\arcsecond}}
\newcommand*{\ineV}[1]{\unit{#1}{\electronvolt}}
\newcommand*{\ineVocs}[1]{\unit{#1}{\mathrm{eV}\per c^2}}
\newcommand*{\ineVoc}[1]{\unit{#1}{\mathrm{eV}\per c}}
@@ -349,11 +355,11 @@
\newphysicsquantity{planeangle}%
{\m\usk\reciprocal\m}%
[\rad]%
- []
+ [\rad]
\newphysicsquantity{solidangle}%
{\m\squared\usk\reciprocalsquare\m}%
[\sr]%
- []
+ [\sr]
\newphysicsquantity{velocity}%
{\m\usk\reciprocal\s}%
[\m\usk\reciprocal\s]%
@@ -716,6 +722,7 @@
{\newcommand*{\dirvect}[1]{\ensuremath{\widehat{#1}}}}}
\newcommand*{\direction}[1]{\ensuremath{\mivector{#1}}}
\newcommand*{\vectordirection}{\direction}
+\newcommand*{\factorvect}[1]{\magvect{#1}\dirvect{#1}}
\newcommand*{\componentalong}[2]{\ensuremath{\mathrm{comp}_{#1}{#2}}}
\newcommand*{\expcomponentalong}[2]{\ensuremath{\frac{\vectdotvect{#2}{#1}}
{\magof{#1}}}}
@@ -815,7 +822,6 @@
\ifthenelse{\boolean{@optromanvectors}}
{\newcommand*{\dirvectsub}[2]{\ensuremath{\ssub{\widehat{\mathrm{#1}}}{#2}}}}
{\newcommand*{\dirvectsub}[2]{\ensuremath{\ssub{\widehat{#1}}{#2}}}}
-\newcommand*{\directionsub}{\dirvectsub}
\newcommand*{\dvectsub}[2]{\ensuremath{\mathrm{d}\vectsub{#1}{#2}}}
\newcommand*{\Dvectsub}[2]{\ensuremath{\Delta\vectsub{#1}{#2}}}
\newcommand*{\compdvectsub}[3]{\ensuremath{\mathrm{d}\compvectsub{#1}{#2}{#3}}}
@@ -847,14 +853,18 @@
\compDervectsub{#1}{#2}{x}{#3},%
\compDervectsub{#1}{#2}{y}{#3},%
\compDervectsub{#1}{#2}{z}{#3}\rv}}
-\newcommand*{\vectdotvect}[2]{\ensuremath{{#1}\bullet{#2}}}
-\newcommand*{\vectdotsvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsvect{#2}}}
+\newcommand*{\vectdotvect}[2]{\ensuremath{{#1}\cdot{#2}}}
+\newcommand*{\vectDotvect}[2]{\ensuremath{{#1}\bullet{#2}}}
+\newcommand*{\vectdotsvect}[2]{\ensuremath{\scompsvect{#1}\cdot\scompsvect{#2}}}
+\newcommand*{\vectDotsvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsvect{#2}}}
\newcommand*{\vectdotevect}[2]{\ensuremath{%
\compvect{#1}{x}\compvect{#2}{x}+%
\compvect{#1}{y}\compvect{#2}{y}+%
\compvect{#1}{z}\compvect{#2}{z}}}
-\newcommand*{\vectdotsdvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsdvect{#2}}}
-\newcommand*{\vectdotsDvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsDvect{#2}}}
+\newcommand*{\vectdotsdvect}[2]{\ensuremath{\scompsvect{#1}\cdot\scompsdvect{#2}}}
+\newcommand*{\vectDotsdvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsdvect{#2}}}
+\newcommand*{\vectdotsDvect}[2]{\ensuremath{\scompsvect{#1}\cdot\scompsDvect{#2}}}
+\newcommand*{\vectDotsDvect}[2]{\ensuremath{\scompsvect{#1}\bullet\scompsDvect{#2}}}
\newcommand*{\vectdotedvect}[2]{\ensuremath{%
\compvect{#1}{x}\compdvect{#2}{x}+%
\compvect{#1}{y}\compdvect{#2}{y}+%
@@ -864,6 +874,8 @@
\compvect{#1}{y}\compDvect{#2}{y}+%
\compvect{#1}{z}\compDvect{#2}{z}}}
\newcommand*{\vectsubdotsvectsub}[4]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsvectsub{#3}{#4}}}
+\newcommand*{\vectsubDotsvectsub}[4]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsvectsub{#3}{#4}}}
\newcommand*{\vectsubdotevectsub}[4]{\ensuremath{%
\compvectsub{#1}{#2}{x}\compvectsub{#3}{#4}{x}+%
@@ -870,8 +882,12 @@
\compvectsub{#1}{#2}{y}\compvectsub{#3}{#4}{y}+%
\compvectsub{#1}{#2}{z}\compvectsub{#3}{#4}{z}}}
\newcommand*{\vectsubdotsdvectsub}[4]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsdvectsub{#3}{#4}}}
+\newcommand*{\vectsubDotsdvectsub}[4]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsdvectsub{#3}{#4}}}
\newcommand*{\vectsubdotsDvectsub}[4]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsDvectsub{#3}{#4}}}
+\newcommand*{\vectsubDotsDvectsub}[4]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsDvectsub{#3}{#4}}}
\newcommand*{\vectsubdotedvectsub}[4]{\ensuremath{%
\compvectsub{#1}{#2}{x}\compdvectsub{#3}{#4}{x}+%
@@ -882,8 +898,12 @@
\compvectsub{#1}{#2}{y}\compDvectsub{#3}{#4}{y}+%
\compvectsub{#1}{#2}{z}\compDvectsub{#3}{#4}{z}}}
\newcommand*{\vectsubdotsdvect}[3]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsdvect{#3}}}
+\newcommand*{\vectsubDotsdvect}[3]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsdvect{#3}}}
\newcommand*{\vectsubdotsDvect}[3]{\ensuremath{%
+ \scompsvectsub{#1}{#2}\cdot\scompsDvect{#3}}}
+\newcommand*{\vectsubDotsDvect}[3]{\ensuremath{%
\scompsvectsub{#1}{#2}\bullet\scompsDvect{#3}}}
\newcommand*{\vectsubdotedvect}[3]{\ensuremath{%
\compvectsub{#1}{#2}{x}\compdvect{#3}{x}+%
@@ -894,8 +914,12 @@
\compvectsub{#1}{#2}{y}\compDvect{#3}{y}+%
\compvectsub{#1}{#2}{z}\compDvect{#3}{z}}}
\newcommand*{\dervectdotsvect}[3]{\ensuremath{%
+ \scompsdervect{#1}{#2}\cdot\scompsvect{#3}}}
+\newcommand*{\dervectDotsvect}[3]{\ensuremath{%
\scompsdervect{#1}{#2}\bullet\scompsvect{#3}}}
\newcommand*{\Dervectdotsvect}[3]{\ensuremath{%
+ \scompsDervect{#1}{#2}\cdot\scompsvect{#3}}}
+\newcommand*{\DervectDotsvect}[3]{\ensuremath{%
\scompsDervect{#1}{#2}\bullet\scompsvect{#3}}}
\newcommand*{\dervectdotevect}[3]{\ensuremath{%
\compdervect{#1}{x}{#2}\compvect{#3}{x}+%
@@ -906,8 +930,12 @@
\compDervect{#1}{y}{#2}\compvect{#3}{y}+%
\compDervect{#1}{z}{#2}\compvect{#3}{z}}}
\newcommand*{\vectdotsdervect}[3]{\ensuremath{%
+ \scompsvect{#1}\cdot\scompsdervect{#2}{#3}}}
+\newcommand*{\vectDotsdervect}[3]{\ensuremath{%
\scompsvect{#1}\bullet\scompsdervect{#2}{#3}}}
\newcommand*{\vectdotsDervect}[3]{\ensuremath{%
+ \scompsvect{#1}\cdot\scompsDervect{#2}{#3}}}
+\newcommand*{\vectDotsDervect}[3]{\ensuremath{%
\scompsvect{#1}\bullet\scompsDervect{#2}{#3}}}
\newcommand*{\vectdotedervect}[3]{\ensuremath{%
\compvect{#1}{x}\compdervect{#2}{x}{#3}+%
@@ -918,8 +946,12 @@
\compvect{#1}{y}\compDervect{#2}{y}{#3}+%
\compvect{#1}{z}\compDervect{#2}{z}{#3}}}
\newcommand*{\dervectdotsdvect}[3]{\ensuremath{%
+ \scompsdervect{#1}{#2}\cdot\scompsdvect{#3}}}
+\newcommand*{\dervectDotsdvect}[3]{\ensuremath{%
\scompsdervect{#1}{#2}\bullet\scompsdvect{#3}}}
\newcommand*{\DervectdotsDvect}[3]{\ensuremath{%
+ \scompsDervect{#1}{#2}\cdot\scompsDvect{#3}}}
+\newcommand*{\DervectDotsDvect}[3]{\ensuremath{%
\scompsDervect{#1}{#2}\bullet\scompsDvect{#3}}}
\newcommand*{\dervectdotedvect}[3]{\ensuremath{%
\compdervect{#1}{x}{#2}\compdvect{#3}{x}+%
@@ -936,8 +968,12 @@
\newcommand*{\rtriplecross}[3]{\ensuremath{{#1}\boldsymbol{\times}%
\inparens{{#2}\boldsymbol{\times}{#3}}}}
\newcommand*{\ltriplescalar}[3]{\ensuremath{%
+ {#1}\boldsymbol{\times}{#2}\cdot{#3}}}
+\newcommand*{\ltripleScalar}[3]{\ensuremath{%
{#1}\boldsymbol{\times}{#2}\bullet{#3}}}
\newcommand*{\rtriplescalar}[3]{\ensuremath{%
+ {#1}\cdot{#2}\boldsymbol{\times}{#3}}}
+\newcommand*{\rtripleScalar}[3]{\ensuremath{%
{#1}\bullet{#2}\boldsymbol{\times}{#3}}}
\newcommand*{\ezero}{\ensuremath{\boldsymbol{e}_0}}
\newcommand*{\eone}{\ensuremath{\boldsymbol{e}_1}}
@@ -1146,7 +1182,7 @@
\left\lvert{#2}\right\rangle}}
\newphysicsconstant{oofpez}%
{\ensuremath{\frac{1}{\phantom{_o}4\pi\epsilon_0}}}%
- {\mi at p{9}{8.9876}\timestento{9}}%
+ {\mi at p{9}{8.9875517873681764}\timestento{9}}%
{\m\cubed\usk\kg\usk\reciprocalquartic\s\usk\A\reciprocalsquared}%
[\m\per\farad]%
[\newton\usk\m\squared\per\coulomb\squared]
@@ -1158,7 +1194,7 @@
[\N\usk\s\squared\per\C\squared]
\newphysicsconstant{vacuumpermittivity}%
{\ensuremath{\epsilon_0}}%
- {\mi at p{9.0}{8.8542}\timestento{-12}}%
+ {\mi at p{9.0}{8.854187817}\timestento{-12}}%
{\m\reciprocalcubed\usk\reciprocal\kg\usk\s\quarted\usk\A\squared}%
[\F\per\m]%
[\C\squared\per\N\usk\m\squared]
@@ -1176,103 +1212,103 @@
[\T\usk\m\per\A]
\newphysicsconstant{boltzmann}%
{\ensuremath{k_B}}%
- {\mi at p{1.4}{1.3806}\timestento{-23}}%
+ {\mi at p{1.4}{1.38064852}\timestento{-23}}%
{\m\squared\usk\kg\usk\reciprocalsquare\s\usk\reciprocal\K}%
[\joule\per\K]%
[\J\per\K]
\newphysicsconstant{boltzmannineV}%
{\ensuremath{k_B}}%
- {\mi at p{8.6}{8.6173}\timestento{-5}}%
+ {\mi at p{8.6}{8.6173303}\timestento{-5}}%
{\eV\usk\reciprocal\K}%
[\eV\per\K]%
[\eV\per\K]
\newphysicsconstant{stefanboltzmann}%
{\ensuremath{\sigma}}%
- {\mi at p{5.7}{5.6704}\timestento{-8}}%
+ {\mi at p{5.7}{5.670367}\timestento{-8}}%
{\kg\usk\s\reciprocalcubed\usk\K\reciprocalquarted}%
[\W\per\m\squared\usk\K^4]%
[\W\per\m\squared\usk\K\quarted]
\newphysicsconstant{planck}%
{\ensuremath{h}}%
- {\mi at p{6.6}{6.6261}\timestento{-34}}%
+ {\mi at p{6.6}{6.626070040}\timestento{-34}}%
{\m\squared\usk\kg\usk\reciprocal\s}%
[\J\usk\s]%
[\J\usk\s]
\newphysicsconstant{planckineV}%
{\ensuremath{h}}%
- {\mi at p{4.1}{4.1357}\timestento{-15}}%
+ {\mi at p{4.1}{4.135667662}\timestento{-15}}%
{\eV\usk\s}%
[\eV\usk\s]%
[\eV\usk\s]
\newphysicsconstant{planckbar}%
{\ensuremath{\hslash}}%
- {\mi at p{1.1}{1.0546}\timestento{-34}}%
+ {\mi at p{1.1}{1.054571800}\timestento{-34}}%
{\m\squared\usk\kg\usk\reciprocal\s}%
[\J\usk\s]%
[\J\usk\s]
\newphysicsconstant{planckbarineV}%
{\ensuremath{\hslash}}%
- {\mi at p{6.6}{6.5821}\timestento{-16}}%
+ {\mi at p{6.6}{6.582119514}\timestento{-16}}%
{\eV\usk\s}%
[\eV\usk\s]%
[\eV\usk\s]
\newphysicsconstant{planckc}%
{\ensuremath{hc}}%
- {\mi at p{2.0}{1.9864}\timestento{-25}}%
+ {\mi at p{2.0}{1.98644568}\timestento{-25}}%
{\m\cubed\usk\kg\usk\reciprocalsquare\s}%
[\J\usk\m]%
[\J\usk\m]
\newphysicsconstant{planckcineV}%
{\ensuremath{hc}}%
- {\mi at p{2.0}{1.9864}\timestento{-25}}%
+ {\mi at p{1240}{1.23984193}\timestento{3}}%
{\eV\usk\text{n}\m}%
[\eV\usk\text{n}\m]%
[\eV\usk\text{n}\m]
\newphysicsconstant{rydberg}%
{\ensuremath{\msub{R}{\infty}}}%
- {\mi at p{1.1}{1.0974}\timestento{7}}%
+ {\mi at p{1.1}{1.0973731568508}\timestento{7}}%
{\reciprocal\m}%
[\reciprocal\m]%
[\reciprocal\m]
\newphysicsconstant{bohrradius}%
{\ensuremath{a_0}}%
- {\mi at p{5.3}{5.2918}\timestento{-11}}%
+ {\mi at p{5.3}{5.2917721067}\timestento{-11}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{finestructure}%
{\ensuremath{\alpha}}%
- {\mi at p{\frac{1}{137}}{7.2974\timestento{-3}}}%
+ {\mi at p{\frac{1}{137}}{7.2973525664\timestento{-3}}}%
{}%
[]%
[]
\newphysicsconstant{avogadro}%
{\ensuremath{N_A}}%
- {\mi at p{6.0}{6.0221}\timestento{23}}%
+ {\mi at p{6.0}{6.022140857}\timestento{23}}%
{\reciprocal\mol}%
[\reciprocal\mol]%
[\reciprocal\mol]
\newphysicsconstant{universalgrav}%
{\ensuremath{G}}%
- {\mi at p{6.7}{6.6738}\timestento{-11}}%
+ {\mi at p{6.7}{6.67408}\timestento{-11}}%
{\m\cubed\usk\reciprocal\kg\usk\s\reciprocalsquared}%
[\J\usk\m\per\kg\squared]%
[\N\usk\m\squared\per\kg\squared]
\newphysicsconstant{surfacegravfield}%
{\ensuremath{g}}%
- {\mi at p{9.8}{9.80}}%
+ {\mi at p{9.8}{9.807}}%
{\m\usk\s\reciprocalsquared}%
[\N\per\kg]%
[\N\per\kg]
\newphysicsconstant{clight}%
{\ensuremath{c}}%
- {\mi at p{3}{2.9979}\timestento{8}}%
+ {\mi at p{3}{2.99792458}\timestento{8}}%
{\m\usk\reciprocal\s}%
[\m\per\s]%
[\m\per\s]
\newphysicsconstant{clightinfeet}%
{\ensuremath{c}}%
- {\mi at p{1}{0.9836}}%
+ {\mi at p{1}{0.983571}}%
{\text{ft}\usk\reciprocal{\text{n}\s}}%
[\text{ft}\per\text{n}\s]%
[\text{ft}\per\mathrm{n}\s]
@@ -1284,31 +1320,31 @@
[\m]
\newphysicsconstant{Mproton}%
{\ensuremath{m_p}}%
- {\mi at p{1.7}{1.6726}\timestento{-27}}%
+ {\mi at p{1.7}{1.672621898}\timestento{-27}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{Mneutron}%
{\ensuremath{m_n}}%
- {\mi at p{1.7}{1.6749}\timestento{-27}}%
+ {\mi at p{1.7}{1.674927471}\timestento{-27}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{Mhydrogen}%
{\ensuremath{m_H}}%
- {\mi at p{1.7}{1.6737}\timestento{-27}}%
+ {\mi at p{1.7}{1.6737236}\timestento{-27}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{Melectron}%
{\ensuremath{m_e}}%
- {\mi at p{9.1}{9.1094}\timestento{-31}}%
+ {\mi at p{9.1}{9.10938356}\timestento{-31}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{echarge}%
{\ensuremath{e}}%
- {\mi at p{1.6}{1.6022}\timestento{-19}}%
+ {\mi at p{1.6}{1.6021766208}\timestento{-19}}%
{\A\usk\s}%
[\C]%
[\C]
@@ -1338,61 +1374,61 @@
[\C]
\newphysicsconstant{MEarth}%
{\ensuremath{M_{\text{Earth}}}}%
- {\mi at p{6.0}{5.9736}\timestento{24}}%
+ {\mi at p{6.0}{5.97237}\timestento{24}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{MMoon}%
{\ensuremath{M_{\text{Moon}}}}%
- {\mi at p{7.3}{7.3459}\timestento{22}}%
+ {\mi at p{7.3}{7.342}\timestento{22}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{MSun}%
{\ensuremath{M_{\text{Sun}}}}%
- {\mi at p{2.0}{1.9891}\timestento{30}}%
+ {\mi at p{2.0}{1.98855}\timestento{30}}%
{\kg}%
[\kg]%
[\kg]
\newphysicsconstant{REarth}%
{\ensuremath{R_{\text{Earth}}}}%
- {\mi at p{6.4}{6.3675}\timestento{6}}%
+ {\mi at p{6.4}{6.371}\timestento{6}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{RMoon}%
{\ensuremath{R_{\text{Moon}}}}%
- {\mi at p{1.7}{1.7375}\timestento{6}}%
+ {\mi at p{1.7}{1.7371}\timestento{6}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{RSun}%
{\ensuremath{R_{\text{Sun}}}}%
- {\mi at p{7.0}{6.9634}\timestento{8}}%
+ {\mi at p{7.0}{6.957}\timestento{8}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{ESdist}%
{\magvectsub{r}{ES}}%
- {\mi at p{1.5}{1.4960}\timestento{11}}%
+ {\mi at p{1.5}{1.496}\timestento{11}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{SEdist}%
{\magvectsub{r}{SE}}%
- {\mi at p{1.5}{1.4960}\timestento{11}}%
+ {\mi at p{1.5}{1.496}\timestento{11}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{EMdist}%
{\magvectsub{r}{EM}}%
- {\mi at p{3.8}{3.8440}\timestento{8}}%
+ {\mi at p{3.8}{3.81550}\timestento{8}}%
{\m}%
[\m]%
[\m]
\newphysicsconstant{MEdist}%
{\magvectsub{r}{ME}}%
- {\mi at p{3.8}{3.8440}\timestento{8}}%
+ {\mi at p{3.8}{3.81550}\timestento{8}}%
{\m}%
[\m]%
[\m]
@@ -1501,6 +1537,7 @@
\newcommand*{\sumoverall}[1]{\ensuremath{\displaystyle
\sum_{\substack{\text{\tiny{all }}\text{\tiny{{#1}}}}}}}
\newcommand*{\dx}[1]{\ensuremath{\,\mathrm{d}{#1}}}
+\newcommand*{\dslashx}[1]{\ensuremath{\,\mathchar'26\mkern-12mu \mathrm{d}{#1}}}
\newcommandx{\evaluatedfromto}[2][2,usedefault]{\ensuremath{%
\Bigg.\Bigg\rvert_{#1}^{#2}}}
\newcommand*{\evaluatedat}{\evaluatedfromto}
@@ -1603,6 +1640,7 @@
\newcommand*{\scripty}[1]{\ensuremath{\mathcalligra{#1}}}
\newcommand*{\Lagr}{\ensuremath{\mathcal{L}}}
\newcommandx{\flux}[1][1]{\ensuremath{\ssub{\Phi}{#1}}}
+\newcommandx{\circulation}[1][1]{\ensuremath{\ssub{\Gamma}{#1}}}
\newcommand*{\absof}[1]{\ensuremath{%
\left\lvert{\ifblank{#1}{\:\_\:}{#1}}\right\rvert}}
\newcommand*{\inparens}[1]{\ensuremath{%
@@ -1631,12 +1669,12 @@
\newcommand*{\hms}[3]{\ensuremath{%
{#1}^{\hour}{#2}^{\mathrm{m}}{#3}^{\s}}}
\newcommand*{\clockreading}{\hms}
-\newcommand*{\latitude}[1]{\unit{#1}{\degree}}
-\newcommand*{\latitudeN}[1]{\unit{#1}{\degree\;\mathrm{N}}}
-\newcommand*{\latitudeS}[1]{\unit{#1}{\degree\;\mathrm{S}}}
-\newcommand*{\longitude}[1]{\unit{#1}{\degree}}
-\newcommand*{\longitudeE}[1]{\unit{#1}{\degree\;\mathrm{E}}}
-\newcommand*{\longitudeW}[1]{\unit{#1}{\degree\;\mathrm{W}}}
+\newcommand*{\latitude}[1]{\unit{#1}{\mkern-\thickmuskip\degree}}
+\newcommand*{\latitudeN}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{N}}}
+\newcommand*{\latitudeS}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{S}}}
+\newcommand*{\longitude}[1]{\unit{#1}{\mkern-\thickmuskip\degree}}
+\newcommand*{\longitudeE}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{E}}}
+\newcommand*{\longitudeW}[1]{\unit{#1}{\mkern-\thickmuskip\degree\;\mathrm{W}}}
\newcommand*{\ssub}[2]{\ensuremath{#1_{\text{#2}}}}
\newcommand*{\ssup}[2]{\ensuremath{#1^{\text{#2}}}}
\newcommand*{\ssud}[3]{\ensuremath{#1^{\text{#2}}_{\text{#3}}}}
@@ -1736,8 +1774,8 @@
\mivector{\_ , \_ , \_}}{#4}}}\times{{\ifblank{#5}{\mivector{\_ , \_ , \_}}{#5}}}}}
\newcommand*{\springinteractionplaces}[3]{\ensuremath{\inparens{#1}
\inparens{#2}{{\ifblank{#3}{\mivector{\_ , \_ , \_}}{#3}}}}}
-\newcommand*{\gravitationalpotentialenergyplaces}[3]{%
- -\genericpotentialenergyplaces{\universalgrav}{#1}{#2}{#3}}
+\newcommand*{\gravitationalpotentialenergyplaces}[3]{\ensuremath{%
+ -\genericpotentialenergyplaces{\universalgrav}{#1}{#2}{#3}}}
\newcommand*{\electricpotentialenergyplaces}[3]{%
\genericpotentialenergyplaces{\oofpez}{#1}{#2}{#3}}
\newcommand*{\springpotentialenergyplaces}[2]{\ensuremath{%
@@ -2272,6 +2310,21 @@
\end{align*}
\end{mdframed}
}%
+\mdfdefinestyle{mistandardstyle}{%
+ hidealllines=false,skipbelow=\baselineskip,skipabove=\baselineskip,
+ leftmargin=40pt,rightmargin=40pt,linewidth=1,roundcorner=10,
+ nobreak=true,
+ frametitle={STANDARD},
+ frametitlebackgroundcolor=cyan!60,frametitlerule=true,frametitlerulewidth=1,
+ backgroundcolor=cyan!25,
+ linecolor=black,fontcolor=black,shadow=true}
+\NewEnviron{mistandard}{%
+ \begin{mdframed}[style=mistandardstyle]
+ \begin{adjactivityanswer}[cyan!25][cyan!25][black]
+ \BODY
+ \end{adjactivityanswer}
+ \end{mdframed}
+}%
\mdfdefinestyle{bwinstructornotestyle}{%
hidealllines=false,skipbelow=\baselineskip,skipabove=\baselineskip,
leftmargin=40pt,rightmargin=40pt,linewidth=1,roundcorner=10,
@@ -2326,6 +2379,21 @@
\end{align*}
\end{mdframed}
}%
+\mdfdefinestyle{bwstandardstyle}{%
+ hidealllines=false,skipbelow=\baselineskip,skipabove=\baselineskip,
+ leftmargin=40pt,rightmargin=40pt,linewidth=1,roundcorner=10,
+ nobreak=true,
+ frametitle={STANDARD},
+ frametitlebackgroundcolor=gray!50,frametitlerule=true,frametitlerulewidth=1,
+ backgroundcolor=gray!20,
+ linecolor=black,fontcolor=black,shadow=true}
+\NewEnviron{bwstandard}{%
+ \begin{mdframed}[style=bwstandardstyle]
+ \begin{adjactivityanswer}[gray!20][gray!20][black]
+ \BODY
+ \end{adjactivityanswer}
+ \end{mdframed}
+}%
\NewEnviron{mysolution}{%
\setcounter{equation}{0}
\begin{align}
@@ -2344,20 +2412,23 @@
\newlist{parts}{enumerate}{2}%
\setlist[parts]{label=(\alph*)}}{\newpage}
\newcommand{\problempart}{\item}%
-\newcommand{\reason}[1]{\parbox{2cm}{#1}}
+\newcommand{\reason}[1]{\begin{minipage}{5cm}{#1}\end{minipage}}
\newcommand*{\checkpoint}{%
\vspace{1cm}\begin{center}%
\colorbox{yellow!80}{|--------- CHECKPOINT ---------|}%
\end{center}}%
-\newcommand*{\image}[2]{%
- \begin{figure}[h!]
+\newcommandx*{\image}[4][1={scale=1},usedefault]{%
+ \begin{figure}[H]
\begin{center}%
- \includegraphics[scale=1]{#1}%
- \caption{#2}%
- \label{#1}%
+ \includegraphics[#1]{#2}%
\end{center}%
+ \caption{#3}%
+ \label{#4}%
\end{figure}}
\newcommand*{\sneakyone}[1]{\ensuremath{\cancelto{1}{#1}}}
+\newcommand*{\parallelto}{\ensuremath{{{\mkern3mu\vphantom{\perp}\vrule depth 0pt
+ \mkern2mu\vrule depth 0pt\mkern3mu}}}}
+\newcommand*{\perpendicularto}{\ensuremath{\perp}}
\newcommand*{\qed}{\ensuremath{\text{ Q.E.D.}}}
\newcommand*{\chkquantity}[1]{%
\begin{center}
@@ -2370,11 +2441,13 @@
}%
\newcommand*{\chkconstant}[1]{%
\begin{center}
- \begin{tabular}{C{4cm} C{2cm} C{3cm} C{3cm} C{3cm} C{3cm}}
- name & symbol & value & baseunit & drvdunit & tradunit \tabularnewline
- \cs{#1} & \csname #1mathsymbol\endcsname & \csname #1value\endcsname &
- \csname #1onlybaseunit\endcsname & \csname #1onlydrvdunit\endcsname &
- \csname #1onlytradunit\endcsname
+ \begin{tabular}{C{4cm} C{4cm} C{4cm}}
+ name & symbol & value \tabularnewline
+ \cs{#1} & \csname #1mathsymbol\endcsname & \csname #1value\endcsname
+ \tabularnewline
+ baseunit & drvdunit & tradunit \tabularnewline
+ \csname #1onlybaseunit\endcsname & \csname #1onlydrvdunit\endcsname &
+ \csname #1onlytradunit\endcsname
\end{tabular}
\end{center}
}%
More information about the tex-live-commits
mailing list