Supergravity and the $b\to s,γ$ decay

dc.creatorde Carlos, B.
dc.creatorCasas, J. A.
dc.date1995-09-26
dc.date.accessioned2026-07-07T03:58:15Z
dc.date.available2026-07-07T03:58:15Z
dc.descriptionWe evaluate the branching ratio BR($b\rightarrow s,γ$) in the minimal supersymmetric standard model (MSSM), determining the corresponding phenomenological restrictions on two attractive supergravity scenarios, namely minimal supergravity and a class of models with a natural solution to the $μ$ problem. We have included in the calculation some one--loop refinements that have a substantial impact on the results. It is stressed the fact that an eventual improvement of the experimental bounds of order $10^{-4}$ would strengthen the restrictions on the MSSM dramatically. This would be enough to discard these supergravity scenarios with $μ<0$ if no discrepancy is found with the standard model prediction, while for $μ>0$ there will remain low-energy windows.
dc.description7 pages, latex+sprocl.sty (appended at the end), 4 figures uuencoded. Based on a talk given by B. de Carlos at the International Workshop on Elementary Particle Physics: Present and Future, Valencia (Spain) 5-9 June 1995
dc.identifierhttps://arxiv.org/abs/hep-ph/9509394
dc.identifierhttp://arxiv.org/abs/hep-ph/9509394
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45732
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSupergravity and the $b\to s,γ$ decay
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