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Neutrino mixing in the $\mu\nu$SSM
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abstract
Recently, several reactor oscillation experiments have successively measured a nonzero value for the neutrino mixing angle ${\theta_{13}}$, which is greater than 5 standard deviations. Within framework of the $\mu$ from $\nu$ Supersymmetric Standard Model ($\mu\nu$SSM), three tiny neutrino masses are generated at the tree level through TeV scale seesaw mechanism. In this work, we analyze the neutrino masses and mixing in the $\mu\nu$SSM with a "top down" method, assuming neutrino mass spectrum with normal ordering (NO) or inverted ordering (IO).
Forward citations
Cited by 2 Pith papers
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$B_s^0 \rightarrow \mu^+ \mu^-$ in a flavor violating extension of MSSM
The mu-from-nu SSM can reproduce the measured B_s^0 -> mu+ mu- branching ratio while also satisfying the Bbar -> X_s gamma constraint, for certain ranges of At, kappa, upsilon_nu^c, and A_lambda.
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$B \to X_{\mathrm{s}} l^{+} l^{-}$ in the $\mu$ from $\nu$ Supersymmetric Standard Model
In the μνSSM, B→X_s l+l− is dominated by charged-Higgs C7 in the low-q² region and C9/C10 Z-penguins in the high-q² region, with the forward-backward asymmetry set by C7C10 and C9C10 interference.
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