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Spontaneous Leptogenesis in Higgs Inflation

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arxiv 2010.07563 v3 pith:OBQ45JY5 submitted 2020-10-15 hep-ph gr-qchep-th

classification hep-phgr-qchep-th
keywords higgsinflationleptonnumberasymmetryfieldleptogenesisreheating
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We propose a scenario of spontaneous leptogenesis in Higgs inflation with help from two additional operators: the Weinberg operator (Dim 5) and the derivative coupling of the Higgs field and the current of lepton number (Dim 6). The former is responsible for lepton number violation and the latter induces chemical potential for lepton number. The period of rapidly changing Higgs field, naturally realized in Higgs inflation during the reheating, allows large enhancement in the produced asymmetry in lepton number, which is eventually converted into baryon asymmetry of the universe. This scenario is compatible with high reheating temperature of Higgs inflation model.

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  1. Genesis--Starobinsky inflation can explain the ACT data

    gr-qc 2025-09 conditional novelty 6.0 of 10

    A Genesis-to-Starobinsky inflation model in Horndeski gravity shifts the scalar spectral index upward enough to bring Starobinsky inflation into agreement with ACT CMB data.

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