Supersymmetry parameter analysis: SPA convention and project
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Supersymmetry parameter analysis: SPA convention and project

Juan Antonio Aguilar Saavedra,A. Ali,Benjamin Allanach,R. Arnowitt,H. A. Baer,J. A. Bagger,Csaba Balazs,V. Barger,M. Barnett,A. Bartl,M. Battaglia,P. Bechtle,G. Bélanger,Alexander Belyaev,E. L. Berger,G. Blair,E. Boos,M. Carena,S. Y. Choi,F. Deppisch,A. De Roeck,K. Desch,M. A. Diaz,A. Djouadi,B. Dutta,S. Dutta,H. Eberl,J. Ellis,Jens Erler,H. Fraas,A. Freitas,T. Fritzsche,R. M. Godbole,G. J. Gounaris,Jaume Guasch,J. Gunion,N. Haba,H. E. Haber,K. Hagiwara,L. Han,Tao Han,H.-J. He,S. Heinemeyer,S. Hesselbach,K. Hidaka,I. Hinchliffe,Martin Hirsch,K. Hohenwarter-Sodek,W. Hollik,W. S. Hou,T. Hurth,I. Jack,Y. Jiang,D. R. T. Jones,Jan Kalinowski,T. Kamon,G. Kane,S. K. Kang,T. Kernreiter,W. Kilian,Choong Sun Kim,Stephen King,O. Kittel,M. Klasen,J.-L. Kneur,K. Kovarik,M. Krämer,S. Kraml,Remi Lafaye,Paul Langacker,H. E. Logan,W.-G. Ma,W. Majerotto,H.-U. Martyn,K. Matchev,David Miller,M. Mondragon,G. Moortgat-Pick,S. Moretti,T. Mori,G. Moultaka,S. Muanza,M. M. Mühlleitner,B. Mukhopadhyaya,U. Nauenberg,Mihoko Nojiri,D. Nomura,H. Nowak,N. Okada,Keith Olive,W. Öller,Michael Peskin,T. Plehn,G. Polesello,W. Porod,F. Quevedo,David Rainwater,J. Reuter,P. Richardson,Krzysztof Rolbiecki,P. Roy,R. Rückl,Heidi Rzehak,P. Schleper,K. Siyeon,Peter Skands,P. Slavich,D. Stöckinger,P. Sphicas,M. Spira,Tim Tait,D. R. Tovey,Jose W.F. Valle,C. E. M. Wagner,Ch Weber,G. Weiglein,P. Wienemann,Z.-Z. Xing,Y. Yamada,J. M. Yang,D. Zerwas,P. M. Zerwas,R.-Y. Zhang,X. Zhang,S.-H. Zhu;Juan Antonio Aguilar Saavedra;A. Ali;Benjamin Allanach;R. Arnowitt;H. A. Baer;J. A. Bagger;Csaba Balazs;V. Barger;M. Barnett;A. Bartl;M. Battaglia;P. Bechtle;G. Bélanger;Alexander Belyaev;E. L. Berger;G. Blair;E. Boos;M. Carena;S. Y. Choi;F. Deppisch;A. De Roeck;K. Desch;M. A. Diaz;A. Djouadi;B. Dutta;S. Dutta;H. Eberl;J. Ellis;Jens Erler;H. Fraas;A. Freitas;T. Fritzsche;R. M. Godbole;G. J. Gounaris;Jaume Guasch;J. Gunion;N. Haba;H. E. Haber;K. Hagiwara;L. Han;Tao Han;H.-J. He;S. Heinemeyer;S. Hesselbach;K. Hidaka;I. Hinchliffe;Martin Hirsch;K. Hohenwarter-Sodek;W. Hollik;W. S. Hou;T. Hurth;I. Jack;Y. Jiang;D. R. T. Jones;Jan Kalinowski;T. Kamon;G. Kane;S. K. Kang;T. Kernreiter;W. Kilian;Choong Sun Kim;Stephen King;O. Kittel;M. Klasen;J.-L. Kneur;K. Kovarik;M. Krämer;S. Kraml;Remi Lafaye;Paul Langacker;H. E. Logan;W.-G. Ma;W. Majerotto;H.-U. Martyn;K. Matchev;David Miller;M. Mondragon;G. Moortgat-Pick;S. Moretti;T. Mori;G. Moultaka;S. Muanza;M. M. Mühlleitner;B. Mukhopadhyaya;U. Nauenberg;Mihoko Nojiri;D. Nomura;H. Nowak;N. Okada;Keith Olive;W. Öller;Michael Peskin;T. Plehn;G. Polesello;W. Porod;F. Quevedo;David Rainwater;J. Reuter;P. Richardson;Krzysztof Rolbiecki;P. Roy;R. Rückl;Heidi Rzehak;P. Schleper;K. Siyeon;Peter Skands;P. Slavich;D. Stöckinger;P. Sphicas;M. Spira;Tim Tait;D. R. Tovey;Jose W.F. Valle;C. E. M. Wagner;Ch Weber;G. Weiglein;P. Wienemann;Z.-Z. Xing;Y. Yamada;J. M. Yang;D. Zerwas;P. M. Zerwas;R.-Y. Zhang;X. Zhang;S.-H. Zhu;
the european physical journal c 2006 Vol. 46 pp. 43-60
139
zhu2006thesupersymmetry

Abstract

High-precision analyses of supersymmetry parameters aim at reconstructing the fundamental supersymmetric theory and its breaking mechanism. A well defined theoretical framework is needed when higher-order corrections are included. We propose such a scheme, Supersymmetry Parameter Analysis SPA, based on a consistent set of conventions and input parameters. A repository for computer programs is provided which connect parameters in different schemes and relate the Lagrangian parameters to physical observables at LHC and high energy e + e - linear collider experiments, i.e., masses, mixings, decay widths and production cross sections for supersymmetric particles. In addition, programs for calculating high-precision low energy observables, the density of cold dark matter (CDM) in the universe as well as the cross sections for CDM search experiments are included. The SPA scheme still requires extended efforts on both the theoretical and experimental side before data can be evaluated in the future at the level of the desired precision. We take here an initial step of testing the SPA scheme by applying the techniques involved to a specific supersymmetry reference point.

Keywords

dark matter cdm supersymmetric computer programs supersymmetry parameter analysis spa scheme

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DOI:
10.1140/epjc/s2005-02460-1
URL:
https://sciprofiles.com/publication/view/a2664c854...

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