Gravitational wave signatures of dark sector portal leptogenesis

Fuente: arXiv
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Main Authors: Borah, Debasish, Mahanta, Devabrat, Saha, Indrajit
Format: Preprint
Published: 2025
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author Borah, Debasish
Mahanta, Devabrat
Saha, Indrajit
author_facet Borah, Debasish
Mahanta, Devabrat
Saha, Indrajit
contents We study the possibility of probing leptogenesis via stochastic gravitational waves (GW) arising from a dark sector assisted first-order electroweak phase transition. The same dark sector, with non-trivial transformation under an unbroken $Z_2$ symmetry is also responsible for providing the only source of CP asymmetry via one-loop interference with the tree level decay of a heavy right-handed neutrino into lepton and Higgs doublets. The new Yukawa and scalar portal couplings enhance the CP asymmetry allowing TeV scale leptogenesis without any resonant enhancement. Light neutrino masses arise from a combination of type-I and one-loop contributions with vanishing lightest neutrino mass. While the new degrees of freedom in sub-TeV range keep the detection prospects at terrestrial experiments promising, the new scalars enhance the strength of the electroweak phase transition keeping the GW signals within reach of near future experiments like LISA.
format Preprint
id arxiv_https___arxiv_org_abs_2504_14671
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Gravitational wave signatures of dark sector portal leptogenesis
Borah, Debasish
Mahanta, Devabrat
Saha, Indrajit
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We study the possibility of probing leptogenesis via stochastic gravitational waves (GW) arising from a dark sector assisted first-order electroweak phase transition. The same dark sector, with non-trivial transformation under an unbroken $Z_2$ symmetry is also responsible for providing the only source of CP asymmetry via one-loop interference with the tree level decay of a heavy right-handed neutrino into lepton and Higgs doublets. The new Yukawa and scalar portal couplings enhance the CP asymmetry allowing TeV scale leptogenesis without any resonant enhancement. Light neutrino masses arise from a combination of type-I and one-loop contributions with vanishing lightest neutrino mass. While the new degrees of freedom in sub-TeV range keep the detection prospects at terrestrial experiments promising, the new scalars enhance the strength of the electroweak phase transition keeping the GW signals within reach of near future experiments like LISA.
title Gravitational wave signatures of dark sector portal leptogenesis
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2504.14671