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Affleck-Dine leptogenesis scenario for resonant production of sterile neutrino dark matter

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arxiv 2402.11902 v3 pith:MYLZK57U submitted 2024-02-19 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords darkmatterneutrinoscenariosterileleptogenesisproductionaffleck-dine
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abstract

Sterile neutrino is a fascinating candidate for dark matter. In this paper, we examine the Affleck-Dine (AD) leptogenesis scenario generating a large lepton asymmetry, which can induce the resonant production of sterile neutrino dark matter via the Shi-Fuller (SF) mechanism. We also revisit the numerical calculation of the SF mechanism and the constraints from current X-ray and Lyman-$\alpha$ forest observations. We find that the AD leptogenesis scenario can explain the production of sterile neutrino dark matter by incorporating a non-topological soliton with a lepton charge called L-ball. Finally, we discuss an enhancement of second-order gravitational waves at the L-ball decay and investigate the testability of our scenario with future gravitational wave observations.

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  1. Multiple Populations of Same Sterile Neutrino as Dark Matter

    hep-ph 2025-07 conditional novelty 6.0 of 10

    A single sterile neutrino species can be produced by multiple early-universe mechanisms, yielding cold and warm dark matter populations with a two-humped momentum spectrum.

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