000855264 001__ 855264
000855264 003__ SzGeCERN
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000855264 0248_ $$aoai:cds.cern.ch:855264$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$qcerncds:hep-ph
000855264 0247_ $$2DOI$$a10.1016/j.physletb.2006.01.010
000855264 035__ $$9SPIRES$$a6285244
000855264 035__ $$9Inspire$$a687540
000855264 037__ $$9arXiv$$ahep-ph/0507192$$chep-ph
000855264 037__ $$aCERN-PH-TH-2005-131
000855264 037__ $$aUAB-FT-584
000855264 041__ $$aeng
000855264 084__ $$2CERN Library$$aTH-2005-131
000855264 088__ $$aCERN-PH-TH-2005-131
000855264 100__ $$aAntoniadis, Ignatios$$uCERN
000855264 245__ $$aSplitting Extended Supersymmetry
000855264 260__ $$c2006
000855264 269__ $$aGeneva$$bCERN$$c15 Jul 2005
000855264 300__ $$a10 p
000855264 520__ $$aWe show how splitting supersymmetry reconciles a class of intersecting brane models with unification. The gauge sector in these models arises in multiplets of extended supersymmetry while matter states are in N=1 representations. A deformation of the angles between the branes gives large masses to squarks and sleptons, as well as supersymmetry breaking contributions to other string states. The latter generate at one-loop heavy Dirac masses for Winos and gluinos and can induce a mass term for the Higgsino doublets. We find that this scenario is compatible with gauge coupling unification at high scale for both cases where the gauge sector is N=2 and N=4 supersymmetric. Moreover a neutralino, combination of neutral Higgsinos and Binos, is a natural candidate for dark matter.
000855264 520__ $$aWe show how splitting supersymmetry reconciles a class of intersecting brane models with unification. The gauge sector in these models arises in multiplets of extended supersymmetry while matter states are in N=1 representations. A deformation of the angles between the branes gives large masses to squarks and sleptons, as well as supersymmetry breaking contributions to other string states. The latter generate at one-loop heavy Dirac masses for Winos and gluinos and can induce a mass term for the Higgsino doublets. We find that this scenario is compatible with gauge coupling unification at high scale for both cases where the gauge sector is N=2 and N=4 supersymmetric. Moreover a neutralino, combination of neutral Higgsinos and Binos, is a natural candidate for dark matter.
000855264 520__ $$9Elsevier$$aWe show how splitting supersymmetry reconciles a class of intersecting brane models with unification. The gauge sector in these models arises in multiplets of extended supersymmetry while matter states are in N=1 representations. A deformation of the angles between the branes gives large masses to squarks and sleptons, as well as supersymmetry breaking contributions to other string states. The latter generate at one-loop heavy Dirac masses for winos and gluinos and can induce a mass term for the higgsino doublets. We find that this scenario is compatible with gauge coupling unification at high scale for both cases where the gauge sector is N=2 and N=4 supersymmetric. Moreover a neutralino, combination of neutral higgsinos and binos, is a natural candidate for dark matter.
000855264 542__ $$fElsevier B.V.
000855264 595__ $$aCERN-TH
000855264 595__ $$aLANL EDS
000855264 595__ $$aOA
000855264 595__ $$aSIS:2006 PR/LKR added
000855264 595__ $$aSIS SCIENCEDIR2006
000855264 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
000855264 690C_ $$aARTICLE
000855264 690C_ $$aCERN
000855264 693__ $$aNot applicable$$eNot applicable
000855264 695__ $$9LANL EDS$$aHigh Energy Physics - Phenomenology
000855264 700__ $$aDelgado, Antonio$$uCERN
000855264 700__ $$aBenakli, Karim$$uParis, LPTHE
000855264 700__ $$aQuiros, Mariano$$uICREA, Barcelona$$uBarcelona, IFAE
000855264 700__ $$aTuckmantel, Marc$$uCERN$$uZurich, ETH
000855264 710__ $$5PH-TH
000855264 720__ $$aAntoniadis, Ignatios
000855264 720__ $$aBenakli, Karim
000855264 720__ $$aDelgado, Antonio
000855264 720__ $$aQuiros, Mariano
000855264 720__ $$aTuckmantel, Marc
000855264 773__ $$c302-306$$n2-3$$pPhys. Lett. B$$v634$$y2006
000855264 8564_ $$uhttp://weblib.cern.ch/abstract?CERN-PH-TH-2005-131$$yPreprint
000855264 8564_ $$82437588$$s130611$$uhttp://cds.cern.ch/record/855264/files/arXiv:hep-ph_0507192.pdf
000855264 8564_ $$898053$$s128389$$uhttp://cds.cern.ch/record/855264/files/0507192.pdf$$yAccess to fulltext document
000855264 901__ $$uCERN
000855264 916__ $$sn$$w200529$$ya2006
000855264 960__ $$a13
000855264 961__ $$c20100416$$h0805$$lCER01$$x20050718
000855264 963__ $$aPUBLIC
000855264 970__ $$a002538303CER
000855264 980__ $$aARTICLE