diff --git a/doc/paper.tex b/doc/paper.tex index 187435398..eefdaf62d 100644 --- a/doc/paper.tex +++ b/doc/paper.tex @@ -171,16 +171,16 @@ \section{Program Summary} \section{Introduction} Supersymmetry(SUSY) provides the only non-trivial way to extend the space-time symmetries of the Poincar\'e -group\cite{Coleman:1967ad,Haag:1974qh}, leading many to suspect that +group \cite{Coleman:1967ad,Haag:1974qh}, leading many to suspect that SUSY may be realised in nature in some form. In particular supersymmetric extensions of the standard model where SUSY is broken at the TeV scale have been proposed to solve the hierarchy -problem\cite{Weinberg:1975gm, Weinberg:1979bn, Gildener:1976ai, +problem \cite{Weinberg:1975gm, Weinberg:1979bn, Gildener:1976ai, Susskind:1978ms, 'tHooft:1980xb}, allow gauge coupling -unification\cite{Langacker:1990jh, Ellis:1990wk, Amaldi:1991cn, +unification \cite{Langacker:1990jh, Ellis:1990wk, Amaldi:1991cn, Langacker:1991an, Giunti:1991ta} and predict a dark matter candidate which can fit the observed relic -density\cite{Goldberg:1983nd,Ellis:1983ew}. Such models have also +density \cite{Goldberg:1983nd,Ellis:1983ew}. Such models have also been used for baryogenesis or leptogensis to solve the matter-anti-matter asymmetry of the universe and have been considered as the low energy effective models originating from string @@ -189,7 +189,7 @@ \section{Introduction} Detailed phenomenological studies have been carried out for scenarios within the minimal supersymmetric standard model (MSSM). Such work has been greatly aided by public spectrum generators for -MSSM\cite{Allanach:2001kg,Porod:2003um,Djouadi:2002ze,Baer:1993ae}, +MSSM \cite{Allanach:2001kg,Porod:2003um,Djouadi:2002ze,Baer:1993ae,Chowdhury:2011zr}, allowing fast and reliable exploration of the sparticle spectrum, mixings and couplings, which can be obtained from particular choices of breaking mechanism inspired boundary conditions and specified @@ -239,11 +239,11 @@ \section{Introduction} ideas. \fs is a \mathematica package which uses \sarah to create a fast, modular C++ spectrum generator for a user specified SUSY model. The generated code structure is designed to be as flexible as possible -to accommodate different types of extensions and due to it's modular +to accommodate different types of extensions and due to its modular nature it is easy to modify, add new features and combine with other programs. The generated code has been extensively tested against well -known spectrum generators and as well providing a solution for new -SUSY models the generated MSSM and NMSSM codes offer a modern and fast +known spectrum generators. As well as providing a solution for new +SUSY models, the generated MSSM and NMSSM codes offer a modern and fast alternative to the existing public spectrum generators. In section \ref{Sec:Program} we describe the program in more detail @@ -3075,5 +3075,14 @@ \section*{References} %%CITATION = NUPHA,B178,75;%% %265 citations counted in INSPIRE as of 10 May 2014 +%\cite{Chowdhury:2011zr} +\bibitem{Chowdhury:2011zr} + D.~Chowdhury, R.~Garani and S.~KVempati, + %``SUSEFLAV: Program for supersymmetric mass spectra with seesaw mechanism and rare lepton flavor violating decays,'' + Comput.\ Phys.\ Commun.\ {\bf 184} (2013) 899 + [arXiv:1109.3551 [hep-ph]]. + %%CITATION = ARXIV:1109.3551;%% + %16 citations counted in INSPIRE as of 03 Jun 2014 + \end{thebibliography} \end{document}