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Refined approaches in second leptogenesis for the baryon-lepton asymmetry discrepancy

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arxiv 2406.19694 v2 pith:CM5Q4CQK submitted 2024-06-28 hep-ph astro-ph.CO

Refined approaches in second leptogenesis for the baryon-lepton asymmetry discrepancy

classification hep-ph astro-ph.CO
keywords asymmetryleptogenesismasssecondbaryon-leptondiscrepancyelectroweakheavy
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The temperature-dependent mass of the heavy neutrino can lead to the second leptogenesis occurring below the electroweak scale, potentially explaining the large discrepancy between baryon and lepton asymmetries. We investigate this scenario further, exploring the intricate interplay of the weak interaction processes within this framework. It includes notable shifts in the dominant decay channels of heavy neutrinos around the electroweak symmetry breaking, along with the resonance behavior of the scattering processes near the $W/Z$ mass. The $CP$ asymmetry can also vary over cosmic history due to the temperature-dependent mass, allowing the $B-L$ asymmetry generation to be amplified in the late epoch. These findings elucidate how such alterations in the dynamics of second leptogenesis contribute to addressing the observed discrepancies in baryon-lepton asymmetry.

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  1. Cogenesis of baryon and lepton number asymmetries matching the EMPRESS Data

    hep-ph 2025-09 conditional novelty 5.0

    A U(1)_{B-L} flaton decay chain can produce both a large positive electron-neutrino asymmetry and the observed baryon asymmetry, with values matching EMPRESS and BBN for a symmetry-breaking scale around 10^10 GeV.