The rare radiative decay $B_s \to ν\barν γ$ in beyond Standard Model scenarios

dc.creatorDincer, Yusuf
dc.date2002-04-16
dc.date2003-01-28
dc.date.accessioned2026-07-07T06:32:28Z
dc.date.available2026-07-07T06:32:28Z
dc.descriptionIn this paper, I study the branching ratio of the rare radiative decay $B_s \to ν\barν γ$ in the framework of the Fourth-Generation Standard Model and the Two-Higgs-Doublet Model. It is shown that this quantity is a very effective tool for establishing new physics beyond the Standard Model. It is observed that there is a region in the parameter space in both extensions of the Standard Model for which the branching ratio show considerable departure from the Standard Model.
dc.descriptionThis paper has been withdrawn by the author
dc.identifierhttps://arxiv.org/abs/hep-ph/0204183
dc.identifierhttp://arxiv.org/abs/hep-ph/0204183
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98912
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe rare radiative decay $B_s \to ν\barν γ$ in beyond Standard Model scenarios
dc.typetext

Files

Collections