CERN Accelerating science

000912045 001__ 912045
000912045 003__ SzGeCERN
000912045 005__ 20230131120839.0
000912045 0248_ $$aoai:cds.cern.ch:912045$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$pcerncds:CERN$$qcerncds:hep-ph
000912045 0247_ $$2DOI$$a10.1140/epjc/s2005-02460-1
000912045 035__ $$9SPIRES$$a6443010
000912045 035__ $$9Inspire$$a699194
000912045 037__ $$9arXiv$$ahep-ph/0511344$$chep-ph
000912045 037__ $$aSLAC-PUB-11579
000912045 037__ $$aCERN-PH-TH-2005-232
000912045 037__ $$aDESY-05-242
000912045 037__ $$aFERMILAB-PUB-05-524-T
000912045 037__ $$aKEK-TH-1054
000912045 041__ $$aeng
000912045 084__ $$2CERN Library$$aTH-2005-232
000912045 088__ $$aCERN-PH-TH-2005-232
000912045 088__ $$aDESY-05-242
000912045 088__ $$aDESY-2005-242
000912045 088__ $$aFERMILAB-Pub-2005-524-T
000912045 100__ $$aAguilar-Saavedra, Juan Antonio$$uLisbon, IST
000912045 245__ $$aSupersymmetry Parameter Analysis : SPA Convention and Project
000912045 260__ $$c2006
000912045 269__ $$aGeneva$$bCERN$$c30 Nov 2005
000912045 300__ $$a19 p
000912045 500__ $$9arXiv$$a17pp: references corrected Report-no: CERN-PH-TH/2005-232, DESY 05-242, FERMILAB-PUB-05-524-T, KEK-TH-1054, SLAC-PUB-11579
000912045 520__ $$aHigh-precision analyses of supersymmetry parameters aim at reconstructing the fundamental supersymmetric theory and its breaking mechanism. A well defined theoretical framework is needed when higher-order corrections are included. We propose such a scheme, Supersymmetry Parameter Analysis SPA, based on a consistent set of conventions and input parameters. A repository for computer programs is provided which connect parameters in different schemes and relate the Lagrangian parameters to physical observables at LHC and high energy e+e- linear collider experiments, i.e., masses, mixings, decay widths and production cross sections for supersymmetric particles. In addition, programs for calculating high-precision low energy observables, the density of cold dark matter (CDM) in the universe as well as the cross sections for CDM search experiments are included. The SPA scheme still requires extended efforts on both the theoretical and experimental side before data can be evaluated in the future at the level of the desired precision. We take here an initial step of testing the SPA scheme by applying the techniques involved to a specific supersymmetry reference point.
000912045 520__ $$9Inspire$$aHigh-precision analyses of supersymmetry parameters aim at reconstructing the fundamental supersymmetric theory and its breaking mechanism. A well defined theoretical framework is needed when higher-order corrections are included. We propose such a scheme, Supersymmetry Parameter Analysis SPA, based on a consistent set of conventions and input parameters. A repository for computer programs is provided which connect parameters in different schemes and relate the Lagrangian parameters to physical observables at LHC and high energy e+e- linear collider experiments, i.e., masses, mixings, decay widths and production cross sections for supersymmetric particles. In addition, programs for calculating high-precision low energy observables, the density of cold dark matter (CDM) in the universe as well as the cross sections for CDM search experiments are included. The SPA scheme still requires extended efforts on both the theoretical and experimental side before data can be evaluated in the future at the level of the desired precision. We take here an initial step of testing the SPA scheme by applying the techniques involved to a specific supersymmetry reference point.
000912045 595__ $$aCERN-TH
000912045 595__ $$aLANL EDS
000912045 595__ $$aOA
000912045 595__ $$aSIS:2006 PR/LKR added
000912045 595__ $$aSIS LANLPUBL2006
000912045 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
000912045 690C_ $$aCERN
000912045 690C_ $$aARTICLE
000912045 693__ $$aNot applicable$$eNot applicable
000912045 695__ $$9LANL EDS$$aHigh Energy Physics - Phenomenology
000912045 700__ $$aAli, A.$$uDESY
000912045 700__ $$aAllanach, Benjamin C.$$uCambridge U., DAMTP
000912045 700__ $$aArnowitt, Richard L.$$uTexas A-M
000912045 700__ $$aBaer, Howard A.$$uFlorida State U.
000912045 700__ $$aBagger, Jonathan A.$$uJohns Hopkins U.
000912045 700__ $$aBalazs, Csaba$$uArgonne
000912045 700__ $$aBarger, Vernon D.$$iINSPIRE-00064509$$uWisconsin U., Madison
000912045 700__ $$aBarnett, M.$$uLBL, Berkeley
000912045 700__ $$aBartl, A.$$uVienna U.
000912045 700__ $$aBattaglia, M.$$uLBL, Berkeley
000912045 700__ $$aBechtle, P.$$uSLAC
000912045 700__ $$aBelanger, G.$$uAnnecy, LAPTH
000912045 700__ $$aBelyaev, Alexander$$uMichigan State U.
000912045 700__ $$aBerger, Edmond L.$$uArgonne
000912045 700__ $$aBlair, G.$$uRoyal Holloway, U. of London
000912045 700__ $$aBoos, E.$$uSINP, Moscow
000912045 700__ $$aCarena, Marcela$$uFermilab
000912045 700__ $$aChoi, Seong-Youl$$uChonbuk Natl. U.
000912045 700__ $$aDeppisch, F.$$uDESY
000912045 700__ $$aDe Roeck, A.$$uCERN
000912045 700__ $$aDesch, Klaus$$uFreiburg U.
000912045 700__ $$aDiaz, Marco Aurelio$$uChile U., Catolica
000912045 700__ $$aDjouadi, A.$$uOrsay, LAL
000912045 700__ $$aDutta, Bhaskar$$uTexas A-M
000912045 700__ $$aDutta, Sukanta$$uDelhi U.$$uSLAC
000912045 700__ $$aEberl, Helmut$$uVienna, OAW
000912045 700__ $$aEllis, John R.$$iINSPIRE-00146525$$uCERN
000912045 700__ $$aErler, Jens$$uMexico U.
000912045 700__ $$aFraas, H.$$uWurzburg U.
000912045 700__ $$aFreitas, A.$$uZurich U.
000912045 700__ $$aFritzsche, T.$$uMunich, Max Planck Inst.
000912045 700__ $$aGodbole, R.M.$$uBangalore, Indian Inst. Sci.
000912045 700__ $$aGounaris, G.J.$$uAristotle U., Thessaloniki
000912045 700__ $$aGuasch, Jaume Inglada$$uBarcelona U.
000912045 700__ $$aGunion, John F.$$uUC, Davis
000912045 700__ $$aHaba, N.$$uTokushima U.
000912045 700__ $$aHaber, Howard E.$$uUC, Santa Cruz
000912045 700__ $$aHagiwara, Kaoru$$uKEK, Tsukuba
000912045 700__ $$aHan, L.$$uHefei, CUST
000912045 700__ $$aHan, Tao$$uWisconsin U., Madison
000912045 700__ $$aHe, Hong-Jian$$uTsinghua U., Beijing
000912045 700__ $$aHeinemeyer, Sven$$uCERN
000912045 700__ $$aHesselbach, Stefan$$uUppsala U.
000912045 700__ $$aHidaka, K.$$uTokyo Gakugei U.
000912045 700__ $$aHinchliffe, Ian$$uLBL, Berkeley
000912045 700__ $$aHirsch, Martin$$uValencia U., IFIC
000912045 700__ $$aHohenwarter-Sodek, K.$$uVienna U.
000912045 700__ $$aHollik, W.$$uMunich, Max Planck Inst.
000912045 700__ $$aHou, George W.S.$$uTaiwan, Natl. Taiwan U.
000912045 700__ $$aHurth, T.$$uCERN$$uSLAC
000912045 700__ $$aJack, Ian$$uLiverpool U., Dept. Math.
000912045 700__ $$aJiang, Y.$$uHefei, CUST
000912045 700__ $$aJones, D.R.Timothy$$uLiverpool U., Dept. Math.
000912045 700__ $$aKalinowski, J.$$uWarsaw U.
000912045 700__ $$aKamon, Teruki$$uTexas A-M
000912045 700__ $$aKane, Gordon L.$$uMichigan U., MCTP
000912045 700__ $$aKang, S.K.$$uSeoul Natl. U.
000912045 700__ $$aKernreiter, T.$$uVienna U.
000912045 700__ $$aKilian, Wolfgang$$uDESY
000912045 700__ $$aKim, Choong Sun$$uYonsei U.
000912045 700__ $$aKing, S.F.$$uSouthampton U.
000912045 700__ $$aKittel, Olaf$$uBonn U.
000912045 700__ $$aKlasen, Michael$$uLPSC, Grenoble
000912045 700__ $$aKneur, J.L.$$uMontpellier U.
000912045 700__ $$aKovarik, K.$$uVienna, OAW
000912045 700__ $$aKramer, M.$$qKraemer, M.$$uAachen, Tech. Hochsch.
000912045 700__ $$aKraml, Sabine$$uCERN
000912045 700__ $$aLafaye, R.$$uAnnecy, LAPP
000912045 700__ $$aLangacker, Paul G.$$uPennsylvania U.
000912045 700__ $$aLogan, Heather E.$$uCarleton U.
000912045 700__ $$aMa, W.G.$$uHefei, CUST
000912045 700__ $$aMajerotto, W.$$uVienna, OAW
000912045 700__ $$aMartyn, Hans-Ulrich$$uAachen, Tech. Hochsch.$$uDESY
000912045 700__ $$aMatchev, Konstantin Tzvetanov$$iINSPIRE-00141530$$uFlorida U.
000912045 700__ $$aMiller, D.J.$$iINSPIRE-00107663$$uGlasgow U.
000912045 700__ $$aMondragon, M.$$uMexico U.
000912045 700__ $$aMoortgat-Pick, Gudrid A.$$uCERN
000912045 700__ $$aMoretti, Stefano$$uSouthampton U.
000912045 700__ $$aMori, T.$$uTokyo U., ICEPP
000912045 700__ $$aMoultaka, Gilbert$$uMontpellier U.
000912045 700__ $$aMuanza, S.$$uLyon, IPN
000912045 700__ $$aMuhlleitner, M.M.$$qMuehlleitner, M.M.$$uAnnecy, LAPTH
000912045 700__ $$aMukhopadhyaya, Biswarup$$uHarish-Chandra Res. Inst.
000912045 700__ $$aNauenberg, Uriel$$uColorado U.
000912045 700__ $$aNojiri, Mihoko M.$$uKyoto U., Yukawa Inst., Kyoto
000912045 700__ $$aNomura, Daisuke$$uMichigan State U.
000912045 700__ $$aNowak, H.$$uDESY, Zeuthen
000912045 700__ $$aOkada, Nobuchika$$uKEK, Tsukuba
000912045 700__ $$aOlive, Keith A.$$iINSPIRE-00112984$$uMinnesota U.
000912045 700__ $$aOller, W.$$uVienna, OAW
000912045 700__ $$aPeskin, Michael E.$$iINSPIRE-00115895$$uSLAC
000912045 700__ $$aPlehn, Tilman$$uMunich, Max Planck Inst.
000912045 700__ $$aPolesello, G.$$uINFN, Pavia
000912045 700__ $$aPorod, Werner$$uValencia U., IFIC$$uZurich U.
000912045 700__ $$aQuevedo, Fernando$$uCambridge U., DAMTP
000912045 700__ $$aRainwater, David Landry$$uRochester U.
000912045 700__ $$aReuter, Juergen$$uDESY
000912045 700__ $$aRichardson, Peter$$uDurham U., IPPP
000912045 700__ $$aRolbiecki, K.$$uWarsaw U.
000912045 700__ $$aRoy, P.$$uTata Inst.
000912045 700__ $$aRuckl, Reinhold$$qRueckl, Reinhold$$uWurzburg U.
000912045 700__ $$aRzehak, H.$$uPSI, Villigen
000912045 700__ $$aSchleper, Peter$$uHamburg U.
000912045 700__ $$aSiyeon, Kim$$uChung-Ang U.
000912045 700__ $$aSkands, Peter Z.$$uFermilab
000912045 700__ $$aSlavich, Pietro$$uAnnecy, LAPTH
000912045 700__ $$aStockinger, Dominik$$qStoeckinger, Dominik$$uDurham U., IPPP
000912045 700__ $$aSphicas, Paraskevas$$uCERN
000912045 700__ $$aSpira, Michael$$uPSI, Villigen
000912045 700__ $$aTait, Timothy M.P.$$uArgonne
000912045 700__ $$aTovey, Daniel R.$$uSheffield U.
000912045 700__ $$aValle, Jose W.F.$$iINSPIRE-00133260$$uValencia U., IFIC
000912045 700__ $$aWagner, Carlos E.M.$$iINSPIRE-00134493$$uChicago U., EFI$$uArgonne
000912045 700__ $$aWeber, Ch.$$uVienna, OAW
000912045 700__ $$aWeiglein, Georg$$uDurham U., IPPP
000912045 700__ $$aWienemann, P.$$uFreiburg U.
000912045 700__ $$aXing, Z.Z.$$uBeijing, Inst. High Energy Phys.
000912045 700__ $$aYamada, Y.$$uTohoku U.
000912045 700__ $$aYang, J.M.$$uBeijing, Inst. High Energy Phys.
000912045 700__ $$aZerwas, D.$$uOrsay, LAL
000912045 700__ $$aZerwas, Peter M.$$uDESY
000912045 700__ $$aZhang, R.Y.$$uHefei, CUST
000912045 700__ $$aZhang, X.$$uBeijing, Inst. High Energy Phys.
000912045 700__ $$aZhu, S.H.$$uPeking U.
000912045 710__ $$5PH-TH
000912045 720__ $$aWeber, Ch.
000912045 773__ $$c43-60$$pEur. Phys. J. C$$v46$$y2006
000912045 8564_ $$uhttp://weblib.cern.ch/abstract?CERN-PH-TH-2005-232
000912045 8564_ $$uhttps://lss.fnal.gov/archive/2005/pub/fermilab-pub-05-524-t.pdf$$yFermilab Library Server (fulltext available)
000912045 8564_ $$uhttp://www-public.slac.stanford.edu/sciDoc/docMeta.aspx?slacPubNumber=slac-pub-11579$$ySLAC Document Server
000912045 8564_ $$82326014$$s396568$$uhttp://cds.cern.ch/record/912045/files/arXiv:hep-ph_0511344.pdf
000912045 8564_ $$898539$$s431675$$uhttp://cds.cern.ch/record/912045/files/0511344.pdf$$yAccess to fulltext document
000912045 901__ $$uCERN
000912045 916__ $$sn$$w200548$$ya2006
000912045 960__ $$a13
000912045 961__ $$c20100414$$h0938$$lCER01$$x20051201
000912045 963__ $$aPUBLIC
000912045 970__ $$a002581809CER
000912045 980__ $$aARTICLE