%0 Journal Article %T SuSpect: A Fortran code for the Supersymmetric and Higgs particle spectrum in the MSSM %+ Laboratoire de Physique Théorique et Astroparticules (LPTA) %+ Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT) %A Djouadi, A. %A Kneur, J.-L. %A Moultaka, G. %Z This paper and its associated computer program are available via the Computer Physics Communications homepage on ScienceDirect (http://www.sciencedirect.com/science/journal/00104655) %< avec comité de lecture %@ 0010-4655 %J Computer Physics Communications %I Elsevier %V 176 %P 426-455 %8 2007 %D 2007 %Z hep-ph/0211331 %R 10.1016/j.cpc.2006.11.009 %K Supersymmetry %K Renormalization group equations %K Loop calculations %Z 12.60.Jv; 11.30.Qc; 12.10.-g; 12.15.Lk; 14.80.Cp; 14.80.Ly %Z Physics [physics]/High Energy Physics - Experiment [hep-ex]Journal articles %X We present the Fortran code SuSpect version 2.3, which calculates the Supersymmetric and Higgs particle spectrum in the Minimal Supersymmetric Standard Model (MSSM). The calculation can be performed in constrained models with universal boundary conditions at high scales such as the gravity (mSUGRA), anomaly (AMSB) or gauge (GMSB) mediated supersymmetry breaking models, but also in the non-universal MSSM case with R-parity and CP conservation. Care has been taken to treat important features such as the renormalization group evolution of parameters between low and high energy scales, the consistent implementation of radiative electroweak symmetry breaking and the calculation of the physical masses of the Higgs bosons and supersymmetric particles taking into account the dominant radiative corrections. Some checks of important theoretical and experimental features, such as the absence of non-desired minima, large fine-tuning in the electroweak symmetry breaking condition, as well as agreement with precision measurements can be performed. The program is simple to use, self-contained and can easily be linked to other codes; it is rather fast and flexible, thus allowing scans of the parameter space with several possible options and choices for model assumptions and approximations. %G English %L in2p3-00142888 %U https://hal.in2p3.fr/in2p3-00142888 %~ IN2P3 %~ LPTA %~ CNRS %~ UNIV-MONTP2 %~ UNIV-PSUD %~ UNIV-PARIS-SACLAY %~ UNIV-PSUD-SACLAY %~ UNIV-MONTPELLIER %~ UM1-UM2