% This is a template for a paper, in the format (revtex) needed for submission
% to Physical Review.  It's also a good format for submission to the
% preprint archives.
%
% It's LaTeX, which isn't actually as beautiful and powerful as the
% original TeX language.  One hears that is why Physical Review chose it:
% they like the fact that authors can't write fancy things which confuse
% the printers.  Perhaps that's OK, but LaTeX is still ugly.
%
% I modified this from one of our papers, which probably was modified
% from a previous paper, usw.  It is the preferred method for learning
% the language, as far as I can tell.
%

% Copy this file into your directory.  Copy also the file smiley.ps
% (the PostScript figure included.)

% At the beginning, you will note there are several options.  You can
% print out the document as if it's already been published, buy choosing
% two columns.  Try looking at this document as it already is:
%	latex template_paper.tex
%	latex template_paper.tex
%	xdvi template_paper
% and then changing to two-column style, and looking at it again.  You
% need to latex twice to get the references and equation numbers right, 
% each time you change them.
%
% To see the figure in place, you'll need to produce a PostScript file:
%	latex template_paper.tex
%	dvips template_paper > template_paper.ps
%	ghostview template_paper.ps
%
% To print the paper, you need not save the PostScript, just pipe it
% directly to the printer:
%	latex template_paper.tex
%	dvips template_paper | lpr


%\documentstyle[prl,aps]{revtex}
\documentstyle[preprint,aps]{revtex}

%\documentstyle[12pt][revtex, eqsecnum, twocol]{aps}
%\documentstyle[preprint, revtex, eqsecnum]{aps}

\preprint{\bf PREPRINT}
\input psfig

\begin{document}
\columnsep0.1truecm
\draft
%\preprint{ }
\title{TITLE HERE}
\author{YOUR NAMES}
\address{Physics Department, Cornell University, Ithaca, NY, 14853-2501}
\maketitle

\begin{abstract}
ABSTRACT HERE.

\end{abstract}

\pacs{PACS numbers: 75.60.Ej, 64.60.Ak}

\narrowtext

TEXT HERE.  YOU CAN HAVE REFERENCES\cite{hysterI}, EQUATIONS IN LINE
$E=mc^2$ AND BETWEEN LINES (EQUATION~\ref{curlyD})
\begin{equation}
{\cal D}_{\it int}(s^\sigma (R-R_c)/R) = 
	\lim_{R\to R_c} s^{\tau + \sigma \beta \delta} D_{\it int}(S, R).
\label{curlyD}
\end{equation}


TABLES ARE A MESS (SEE TABLE~\ref{tab:experiments}).

\begin{table}
\begin{tabular}{crl}
\hline
exponents&
\multicolumn{1}{c}{simulation} &
\multicolumn{1}{c}{experiments}\\
&\multicolumn{1}{c}{in 3 dim.} &
\multicolumn{1}{c}{in 3 dimensions}  \\ \hline
$\tau$ &  $1.6\pm0.06$ & 1.74,1.78,1.88; \\
& & $1.5 \pm 0.5$; \\
& & $1.33$; \\
& & $1.5 -1.7$  \\
$\tau+\sigma\beta\delta$&$2.03\pm0.03$ &
1.73-2.1 \\
$(\tau+\sigma\beta\delta-1)/\sigma\nu z +1$&$2.81\pm0.11$&
2.28 \\
$(3-\tau)/ \sigma\nu z$&$2.46\pm0.17$& around
2\\
\hline
\end{tabular}
\vspace{1cm}
\caption
{{\bf Table filled with stuff.}}
\label{tab:experiments}
\end{table}


AND FIGURES CAN BE TRICKY: (SEE FIGURE~\ref{fig:smiley}).

\begin{figure}
\centerline{\psfig{figure=smiley.ps,width=2.0truein}}
\caption{Figure 1: Smiley Face.}
\label{fig:smiley}
\end{figure}

We acknowledge the support of our mothers throughout the years
of our childhood.

\begin{references}

\bibitem{hysterI} J.P.~Sethna, K.~Dahmen, S.~Kartha, J.A.~Krumhansl,
B.W.~Roberts, and J.D.~Shore, {\it Phys. Rev. Lett.} {\bf 70},
3347 (1993); K. Dahmen, S. Kartha, J.A.~Krumhansl, B.W.~Roberts,
J.P.~Sethna, and J.D.~Shore,
{\sl J.~Appl.\ Phys.} {\bf 75}, 5946 (1994).

\end{references}
\end{document}