Baryogenesis via leptogenesis from asymmetric dark matter and radiatively generated neutrino mass

Narendra, Nimmala and Patra, Sudhanwa and Sahu, Narendra and Shil, Sujay (2018) Baryogenesis via leptogenesis from asymmetric dark matter and radiatively generated neutrino mass. Physical Review D, 98 (9). ISSN 2470-0010

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Abstract

We propose an extension of the standard model (SM) by including a dark sector comprised of three generations of heavy right-handed neutrinos, a singlet scalar, and a singlet Dirac fermion, where the latter two particles are stable and are viable candidates of dark matter (DM). In the early Universe, the CP-violating out-of-equilibrium decay of heavy right-handed neutrinos to a singlet Dirac fermion and scalar in the dark sector generates a net DM asymmetry. The latter is then transported to the visible sector via a dimension-eight operator which conserves B - L symmetry and is in thermal equilibrium above the sphaleron decoupling temperature. An additional light singlet scalar is introduced which mixes with the SM Higgs and paves a path for annihilating the symmetric components of the DM candidates. We discuss the constraints on singlet-doublet Higgs mixing from invisible Higgs decay, signal strength at the LHC, and the direct search of DM at terrestrial laboratories. At tree level, the neutrinos are shown to be massless since the symmetry of the dark sector forbids the interaction of right-handed neutrinos with SM particles. However, at the one-loop level, the neutrinos acquire sub-eV masses as required by the oscillation experiments.

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IITH Creators:
IITH CreatorsORCiD
Sahu, NarendraUNSPECIFIED
Item Type: Article
Subjects: Physics
Divisions: Department of Physics
Depositing User: Team Library
Date Deposited: 22 Jan 2019 05:47
Last Modified: 22 Jan 2019 05:47
URI: http://raiith.iith.ac.in/id/eprint/4741
Publisher URL: http://doi.org/10.1103/PhysRevD.98.095016
OA policy: http://www.sherpa.ac.uk/romeo/issn/2470-0010/
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