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Signals of dark matter in a supersymmetric two dark matter model

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arxiv 1012.4007 v2 pith:5JUZZC7G submitted 2010-12-17 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords darkmattermodelneutralinosupersymmetricneutrinoparityabundance
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Supersymmetric radiative neutrino mass models have often two dark matter candidates. One is the usual lightest neutralino with odd R parity and the other is a new neutral particle whose stability is guaranteed by a discrete symmetry that forbids tree-level neutrino Yukawa couplings. If their relic abundance is comparable, dark matter phenomenology can be largely different from the minimal supersymmetric standard model (MSSM). We study this in a supersymmetric radiative neutrino mass model with the conserved R parity and a $Z_2$ symmetry weakly broken by the anomaly effect. The second dark matter with odd parity of this new $Z_2$ is metastable and decays to the neutralino dark matter. Charged particles and photons associated to this decay can cause the deviation from the expected background of the cosmic rays. Direct search of the neutralino dark matter is also expected to show different features from the MSSM since the relic abundance is not composed of the neutralino dark matter only. We discuss the nature of dark matter in this model by analyzing these signals quantitatively.

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  1. Type III Seesaw for Neutrino Masses in $U(1)_{B-L}$ Model with Multi-component Dark Matter

    hep-ph 2019-08 conditional novelty 6.0 of 10

    A new U(1)_{B-L} extension with type III seesaw neutrino mass and two-component fermion dark matter is proposed and constrained by relic density, direct detection, and LHC searches.

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