Thermal leptogenesis, dark matter, and gravitational waves from an extended canonical seesaw scenario
arXiv:2409.08828 · doi:10.1103/w8gl-wbjd
Abstract
In a canonical type-I seesaw scenario, the Standard Model is extended with three singlet right-handed neutrinos (RHNs) with masses to simultaneously explain sub-eV masses of light neutrinos and baryon asymmetry of the Universe at high scales. In this paper, we show that a relatively low-scale thermal leptogenesis accompanied by gravitational wave signatures is possible when the type-I seesaw is extended with a singlet fermion () and a singlet scalar (), where and are odd under a discrete symmetry. We also add a vectorlike fermion doublet and impose a symmetry under which both and are odd while all other particles are even. This gives rise to a singlet-doublet Majorana fermion dark matter in our setup. At a high scale, the symmetry is broken spontaneously by the vacuum expectation value of and leads to (i) mixing between RHNs () and , and (ii) formation of Domain walls (DWs). In the former case, the final lepton asymmetry is generated by the out-of-equilibrium decay of , which dominantly mixes with . We show that the scale of thermal leptogenesis can be lowered to GeV, which is \textit{3} orders of magnitude lower than the thermal leptogenesis in canonical type-I seesaw. In the latter case, the disappearance of the DWs gives observable gravitational wave signatures, which can be probed at LISA, DECIGO, etc.
v2: 15 pages, 9 captioned figures, 3 tables, v3: updated to match the published version in Phys. Rev. D
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- Probing low scale leptogenesis through gravitational wave
- Cogenesis of visible and dark matter in type-I Dirac seesaw
- Impact of conversion-driven processes on singlet-doublet Majorana dark matter relic