Large Cosmological Light Element Bound on R Parity Violating Parameters

dc.creatorKim, Jihn E.
dc.creatorKyae, Bumseok
dc.creatorPark, Jong Dae
dc.date1998-10-28
dc.date1998-11-03
dc.date.accessioned2026-07-07T04:05:35Z
dc.date.available2026-07-07T04:05:35Z
dc.descriptionIn R parity violating theories, there does not exist the {\it stable} lightest supersymmetric particle (LSP). The LSP, $χ$, of MSSM decays to lighter ordinary particles with dimension 6 effective R violating interaction terms. Since the lifetime of $χ$ can be sufficiently long for small R-violating couplings, it can affect the standard nucleosynthesis scenario. This constraint gives an upper limit for the lifetime of $χ$ in the small $τ_χ$ region; $\simτ_χ>10^6$ s. This translates to the sum of squared R-violating couplings, for $m_χ=$ 60 GeV in the photino (bino) limit, $(0.12 (0.05)|λ_{i,j,k}|^2+0.31(0.07) |λ^\prime_{i,j\ne 3,k}|^2 +0.04(0.04)|λ^{\prime}_{i,3,k}|^2 +0.23(0.12)|λ_{i,j,k}^{\prime\prime}(i<j,k\ne 3)|^2)> 7.7\times 10^{-24}$.
dc.description15 pages plus 9 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9810503
dc.identifierhttp://arxiv.org/abs/hep-ph/9810503
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48457
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleLarge Cosmological Light Element Bound on R Parity Violating Parameters
dc.typetext

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