Gravitational wave spectral shapes as a probe of long lived right-handed neutrinos, leptogenesis and dark matter: global versus local B-L cosmic strings
Gravitational wave spectral shapes as a probe of long lived right-handed neutrinos, leptogenesis and dark matter: global versus local B-L cosmic strings
The scale of the seesaw mechanism is typically much larger than the electroweak scale. This hierarchy can be naturally explained by U(1)B−L symmetry, which after spontaneous symmetry breaking, simultaneously generates Majorana masses for neutrinos and produces a network of cosmic strings. Such strings generate a gravitational wave (GW) spectrum which is expected to be almost uniform in frequency unless there is a departure from the usual early radiation domination. We explore this possibility in Type I, II and III seesaw frameworks, finding that only for Type-I, long-lived right-handed neutrinos (RHN) may provide a period of early matter domination for parts of the parameter space, even if they are thermally produced. Such a period leaves distinctive imprints in the GW spectrum in the form of characteristic breaks and a knee feature, arising due to the end and start of the periods of RHN domination. These features, if detected, directly determine the mass M, and effective neutrino mass ˜m of the dominating RHN. We find that GW detectors like LISA and ET could probe RHN masses in the range M ∈ [0.1, 109] GeV and effective neutrino masses in the ˜m ∈ [10−10, 10−8] eV range. We investigate the phenomenological implications of long-lived right-handed neutrinos for both local and global U(1)B−L strings, focusing on dark matter production and leptogenesis. We map the viable and detectable parameter space for successful baryogenesis and asymmetric dark matter production from right-handed neutrino decays. We derive analytical and semi-analytical relations correlating the characteristic gravitational-wave frequencies to the neutrino parameters ˜m and M, as well as to the relic abundances of dark matter and baryons. We find that the detectable parameter space reaches the boundary of hierarchical leptogenesis and encompasses a substantial portion of the near-resonant regime.
astro-ph.CO, hep-ph
Datta, Satyabrata
64fa455c-980a-45d4-a3f3-556f789c7040
Ghoshal, Anish
61e009c4-becc-4864-a59d-e5a52820afe9
Spalding, Angus
62746a0e-b341-46c3-8763-d0820be48ec3
White, Graham
652445c5-e1e5-4ff7-84e1-a3bca45e75d0
Datta, Satyabrata
64fa455c-980a-45d4-a3f3-556f789c7040
Ghoshal, Anish
61e009c4-becc-4864-a59d-e5a52820afe9
Spalding, Angus
62746a0e-b341-46c3-8763-d0820be48ec3
White, Graham
652445c5-e1e5-4ff7-84e1-a3bca45e75d0
[Unknown type: UNSPECIFIED]
Abstract
The scale of the seesaw mechanism is typically much larger than the electroweak scale. This hierarchy can be naturally explained by U(1)B−L symmetry, which after spontaneous symmetry breaking, simultaneously generates Majorana masses for neutrinos and produces a network of cosmic strings. Such strings generate a gravitational wave (GW) spectrum which is expected to be almost uniform in frequency unless there is a departure from the usual early radiation domination. We explore this possibility in Type I, II and III seesaw frameworks, finding that only for Type-I, long-lived right-handed neutrinos (RHN) may provide a period of early matter domination for parts of the parameter space, even if they are thermally produced. Such a period leaves distinctive imprints in the GW spectrum in the form of characteristic breaks and a knee feature, arising due to the end and start of the periods of RHN domination. These features, if detected, directly determine the mass M, and effective neutrino mass ˜m of the dominating RHN. We find that GW detectors like LISA and ET could probe RHN masses in the range M ∈ [0.1, 109] GeV and effective neutrino masses in the ˜m ∈ [10−10, 10−8] eV range. We investigate the phenomenological implications of long-lived right-handed neutrinos for both local and global U(1)B−L strings, focusing on dark matter production and leptogenesis. We map the viable and detectable parameter space for successful baryogenesis and asymmetric dark matter production from right-handed neutrino decays. We derive analytical and semi-analytical relations correlating the characteristic gravitational-wave frequencies to the neutrino parameters ˜m and M, as well as to the relic abundances of dark matter and baryons. We find that the detectable parameter space reaches the boundary of hierarchical leptogenesis and encompasses a substantial portion of the near-resonant regime.
Text
2511.01779v1
- Author's Original
Available under License Other.
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Accepted/In Press date: 3 November 2025
Keywords:
astro-ph.CO, hep-ph
Identifiers
Local EPrints ID: 508642
URI: http://eprints.soton.ac.uk/id/eprint/508642
PURE UUID: ed55d3bf-5e4a-46e7-9766-6a1b12ae4b6a
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Date deposited: 28 Jan 2026 17:59
Last modified: 28 Jan 2026 18:00
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Author:
Satyabrata Datta
Author:
Anish Ghoshal
Author:
Angus Spalding
Author:
Graham White
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