Phenomenology of a New Supersymmetric Standard Model: The $\mu \nu$SSM

Abstract

The $\mu \nu$SSM solves the $\mu$ problem of the MSSM and explains the origin of neutrino masses by simply using right-handed neutrino superfields. The solution implies the breaking of R-parity. The properties and phenomenology of the model are briefly reviewed.

Proceedings of SUSY 2009, 5-10 June, Boston; 4 pages

References in corpus (1)

• Gamma-ray detection from gravitino dark matter decay in the $\mu \nu$SSM

Cited by in corpus (15)

• A 96 GeV Higgs Boson in the N2HDM
• Precise prediction for the Higgs-Boson Masses in the $\mu \nu$SSM
• Radiative contribution to neutrino masses and mixing in $\mu \nu$SSM
• Possible indications for new Higgs bosons in the reach of the LHC: N2HDM and NMSSM interpretations
• Revisiting the SUSY mu problem and its solutions in the LHC era
• The Higgs sector of the munuSSM and collider physics
• Precise prediction for the Higgs-Boson Masses in the $\mu \nu$SSM with three right-handed neutrino superfields
• CLUES on Fermi-LAT prospects for the extragalactic detection of munuSSM gravitino Dark Matter
• Search for sharp and smooth spectral signatures of $\mu \nu$SSM gravitino dark matter with Fermi-LAT
• The $\mu \nu$SSM with an extra U(1)
• munuSSM: A python package for the $\mu$-from-$\nu$ Supersymmetric Standard Model
• Vacuum (meta-)stability in the $\mu \nu$SSM
• Models of Supersymmetry for Dark Matter
• Indirect Dark Matter Searches and Models
• An N2HDM Solution for the possible 96 GeV Excess