revtex
, and
aps
is a mandatory style option for APS authors. Other style options
are eqsecnum
(to number equations by section), preprint
(to
get double-spaced output for submission purposes), tighten
(to get
single-spaced output with the preprint option), and amsfonts
and
amssymb
(for extra font capabilities, see Sec. vii).
There are also style options for each APS journal: pra
, prb
,
prc
, prd
, pre
, prl
, and rmp
for
Physical
Review A, B, C, D, E, Letters,
and Reviews of Modern Physics respectively. pra
is the default. The prb
option gives superscript reference citations, as is the style for
Physical Review B. Other than this, there are no substantial
differences in the journal options. Please do not use the prb
option unless you will be submitting to Physical Review B. The
prl
option yields a slightly different line spacing for
accurate PRL length estimates. The
floats
style option enables LaTeX-style floating figures and
tables---it is not for use with files to be submitted to the
APS. Similarly, the twocolumn style option is for personal use, and
not for use in submitted files.
\documentstyle[aps,pra]{revtex} \begin{document} \draft \title{Title here} \author{Author(s) here} \address{Address(es) here} \author{Another author(s) here} \address{Another address(es) here} \date{\today} \maketitle \begin{abstract} Abstract here. \end{abstract} \pacs{PACS numbers here}Note the
\draft
, \address{#1}
, and \pacs{#1}
commands.
See Sec. vC for details.
floats
option. While floats can be re-enabled by use of the floats
style
option, you cannot use this for files that you submit to the APS;
it is added for your personal use. Floating tables and figures will not
break across pages. All tables expand to fill the column width.
\text{#1}
command will print #1
as regular text
output in math. In particular, you will get hyphens instead of minus signs.
Used in a superscript, you will get the correct size. See Sec.\
vG.
\label{#1}
after \begin{mathletters}
will allow
you to reference the general number of the equations in the
mathletters
environment. For example, if
\begin{mathletters} \label{alleqs} % observe location \begin{equation} E=mc^2,\label{eqa} \end{equation} \begin{equation} E=mc^2,\label{eqb} \end{equation} \begin{equation} E=mc^2,\label{eqc} \end{equation} \end{mathletters}gives the output
then Eq.\ (\ref{alleqs})
gives ``Eq. (3)''.
\bf
command in superscripts, you will get a
correctly sized character.
\tablenote{#1}
, \tablenotetext{#1}
,
and \tablenotemark{#1}
. These commands work in direct analogy to the
regular footnoting commands in LaTeX. They should be used only in
tables, and the notes will come out at the bottom of the table in which
they appear. See apssamp.tex for instructions and examples.
d
in a tabular specification will create a column centered on
the decimal points of the entries. See Sec. vL for details;
see apssamp.tex for examples.
\tensor
(double-headed
overarrow), \overdots
(triple overdots), \overstar
(star),
\overcirc
(circle), \loarrow
(left-going overarrow), and
\roarrow
(right-going overarrow). They scale correctly in
superscripts. See Appendix A for examples.
\case{#1}{#2}
will give text-style fractions (smaller) in
display-style math.
prsty.bst
,
rmp.bst
, that can be used
to prepare bibliographies automatically, as explained in Lamport's book.
\extracolsep{#1}
sets extra intercolumn
spacing, but this extra spacing has already been set in REVTeX to allow
the columns in the table to expand out to fill the text width. Therefore,
\extracolsep{#1}
will not work in REVTeX . Use the @{#1}
command to specify spacing between two adjacent columns, for personal
files. See Appendix C.9.2
of Lamport for a full explanation of @{#1}
. An example has been
given in apssamp.tex. Note that final journal table layout is set by
production software.
\twocolumn
, floats
, etc. You
cannot use these for files that you submit to the APS; they are added for
your personal use. Please let us know of any other incompatibilities.
oldlfont.sty
active. Please let us know if you have any
problems in this area. And don't worry if you don't know what the OFSS and
NFSS are. (See Sec. vii if you are curious.)