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Dark matter asymmetry in supersymmetric Dirac leptogenesis

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arxiv 1211.5409 v1 pith:GFMAJ5L4 submitted 2012-11-23 hep-ph astro-ph.CO

Dark matter asymmetry in supersymmetric Dirac leptogenesis

classification hep-ph astro-ph.CO
keywords darkmattercandidateright-handedsupersymmetricsneutrinoasymmetricdirac
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We discuss asymmetric or symmetric dark matter candidate in the supersymmetric Dirac leptogenesis scenario. By introducing a singlet superfield coupling to right-handed neutrinos, the overabundance problem of dark matter can be evaded and various possibilities for dark matter candidate arise. If the singlino is the lightest supersymmetric particle (LSP), it becomes naturally asymmetric dark matter. On the other hand, the right-handed sneutrino is a symmetric dark matter candidate whose relic density can be determined by the usual thermal freeze-out process. The conventional neutralino or gravitino LSP can be also a dark matter candidate as its non-thermal production from the right-handed sneutrino can be controlled appropriately. In our scenario, the late-decay of heavy supersymmetric particles mainly produce the right-handed sneutrino and neutrino which is harmless to the standard prediction of the big-bang nucleosynthesis.

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