Supersymmetry parameter analysis:: SPA convention and project

被引:234
作者
Aguilar-Saavedra, J. A. [1 ]
Ali, A.
Allanach, B. C.
Arnowitt, R.
Baer, H. A.
Bagger, J. A.
Balazs, C.
Barger, V.
Barnett, M.
Bartl, A.
Battaglia, M.
Bechtle, P.
Belanger, G.
Belyaev, A.
Berger, E. L.
Blair, G.
Boos, E.
Carena, M.
Choi, S. Y.
Deppisch, F.
De Roeckl, A.
Deschl, K.
Diaz, M. A.
Djouadil, A.
Dutta, B.
Dutta, S.
Eberl, H.
Ellis, J.
Erler, J.
Fraas, H.
Freitas, A.
Fritzsche, T.
Godbole, P. M.
Gounaris, G. J.
Guasch, J.
Gunion, J.
Haba, N.
Haber, H. E.
Hagiwara, K.
Han, L.
Hang, T.
He, H. -J.
Heinemeyer, S.
Hesselbach, S.
Hidaka, K.
Hinchliffe, I.
Hirsch, M.
Hohenwarter-Sodekl, K.
Hollik, W.
Hou, W. S.
机构
[1] Inst Super Tecn, Dept Fis, Lisbon, Portugal
[2] Inst Super Tecn, CFTP, Lisbon, Portugal
[3] DESY, D-2000 Hamburg, Germany
[4] Univ Cambridge, DAMTP, Cambridge, England
[5] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
[6] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA
[7] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[8] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA
[9] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[10] Lawrence Berkeley Natl Lab, Berkeley, CA USA
[11] Univ Vienna, Inst Theoret Phys, Vienna, Austria
[12] Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA
[13] Phys Theor Lab, Annecy Le Vieux, France
[14] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[15] Univ London Royal Holloway & Bedford New Coll, Egham TW20 0EX, Surrey, England
[16] MSU, Skobeltsyn Inst Nucl Phys, Moscow, Russia
[17] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[18] Chonbuk Natl Univ, Dept Phys, Chonju, South Korea
[19] CERN, PH Dept, Geneva, Switzerland
[20] Univ Freiburg, Inst Phys, Freiburg, Germany
[21] Pontificia Univ Catolica Chile, Dept Phys, Santiago, Chile
[22] Univ Paris 11, CNRS, LAL, IN2P3, F-91405 Orsay, France
[23] Univ Delhi, Delhi 110007, India
[24] Austrian Acad Sci, Inst Hochenergiephys, A-1050 Vienna, Austria
[25] Univ Nacl Autonoma Mexico, Inst Fis, Mexico City, DF, Mexico
[26] Univ Wurzburg, Inst Theoret Phys & Astrophys, Wurzburg, Germany
[27] Univ Zurich, Inst Theoret Phys, CH-8001 Zurich, Switzerland
[28] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany
[29] Indian Inst Sci, Ctr High Energy Phys, Bangalore 560012, Karnataka, India
[30] Aristotle Univ Thessaloniki, Dept Theoret Phys, GR-54006 Thessaloniki, Greece
[31] Univ Barcelona, Fac Fis, E-08028 Barcelona, Spain
[32] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[33] Univ Tokushima, Inst Theoret Phys, Tokushima 770, Japan
[34] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
[35] KEK, Div Theory, Tsukuba, Ibaraki, Japan
[36] Univ Sci & Technol China, Dept Modern Phys, Hefei 230026, Peoples R China
[37] Tsinghua Univ, Inst Modern Phys, Beijing 100084, Peoples R China
[38] Tsinghua Univ, Ctr High Energy Phys, Beijing 100084, Peoples R China
[39] Uppsala Univ, Uppsala, Sweden
[40] Tokyo Gakugei Univ, Dept Phys, Tokyo, Japan
[41] CSIC, Inst Fis Corpuscular, Valencia, Spain
[42] Natl Taiwan Univ, Dept Phys, Taipei, Taiwan
[43] Univ Liverpool, Dept Math Sci, Liverpool L69 3BX, Merseyside, England
[44] Warsaw Univ, Inst Theoret Phys, Warsaw, Poland
[45] Univ Michigan, MCTP, Ann Arbor, MI 48109 USA
[46] Seoul Natl Univ, Sch Phys, Seoul, South Korea
[47] Yonsei Univ, Dept Phys, Seoul 120749, South Korea
[48] Univ Southampton, Sch Phys & Astron, Southampton, Hants, England
[49] Univ Bonn, Inst Phys, D-5300 Bonn, Germany
[50] Univ Grenoble 1, Lab Phys Subatom & Cosmol, Grenoble, France
来源
EUROPEAN PHYSICAL JOURNAL C | 2006年 / 46卷 / 01期
基金
英国科学技术设施理事会;
关键词
D O I
10.1140/epjc/s2005-02460-1
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
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.
引用
收藏
页码:43 / 60
页数:18
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