DSpace logo

Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/14463
Full metadata record
DC FieldValueLanguage
dc.contributor.authorVaidya, Rishikesh-
dc.date.accessioned2024-02-24T04:48:34Z-
dc.date.available2024-02-24T04:48:34Z-
dc.date.issued2004-11-
dc.identifier.urihttps://arxiv.org/abs/hep-ph/0403148-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14463-
dc.description.abstractWe present a systematic analysis of all the contributions at the leading log order to the branching ratio of the inclusive radiative B decay, B --> X_s + gamma in the framework of supersymmetry without R-parity. The relevant set of four-quark operators involved in QCD running are extended from 6 (within SM and MSSM) to 24, with also many new contributions to the Wilson coefficients of (chromo)magnetic penguins for either chiral structure. We present complete analytical results here without any a priori assumptions on the form of R-parity violation. Mass eigenstate expressions are given, hence the results are free from the commonly adopted mass-insertion approximation. In the numerical analysis, we focus here only on the influence of the trilinear lambda-prime couplings and report on the possibility of a few orders of magnitude improvement for the bounds on a few combinations of the lambda-prime couplings. Our study shows that the Wilson coefficients of the current-current operators due to R-parity violation dominate over the direct contributions to the penguins. However, the inter-play of various contributions is complicated due to the QCD corrections which we elaborate here.en_US
dc.language.isoenen_US
dc.publisherARXIVen_US
dc.subjectPhysicsen_US
dc.subjectHigh Energy Physics - Phenomenology (hep-ph)en_US
dc.subjectSupersymmetryen_US
dc.subjectR-parity Violationen_US
dc.titleRadiative B decays in Supersymmetry without R-parityen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

Files in This Item:
There are no files associated with this item.


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.