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arxiv: 1211.0435 · v2 · pith:OZHAKBYOnew · submitted 2012-11-02 · ✦ hep-ph · astro-ph.CO

Co-genesis of Matter and Dark Matter with Vector-like Fourth Generation Leptons

classification ✦ hep-ph astro-ph.CO
keywords matterdarkfourthgenerationabundancebaryonmassneutrinos
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We propose a simple extension of the standard model by adding a fourth generation vector-like lepton doublet and show that if the fourth neutrino is a massive pseudo-Dirac fermion with mass in the few hundred GeV range and mass splitting of about 100 keV, its lighter component can be a viable inelastic dark matter candidate. Its relic abundance is produced by the CP violating out-of-equilibrium decay of the type-II seesaw scalar triplet, which also gives rise to the required baryon asymmetry of the Universe via type-II leptogenesis, thus providing a simultaneous explanation of dark matter and baryon abundance observed today. Moreover, the induced vacuum expectation value of the same scalar triplet is responsible for the sub-eV Majorana masses to the three active neutrinos. A stable fourth generation of neutrinos is elusive at collider, however might be detected by current dark matter direct search experiments.

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