Minimal multi-majoron model
Minimal multi-majoron model
In order to provide a natural framework for hierarchical right-handed neutrinos, we propose a realistic ultraviolet complete minimal multi-Majoron model (MMMM). We consider two right-handed neutrinos for simplicity, although the model is readily extendable to more. The minimal model introduces two complex scalar Majoron fields ϕ1 and ϕ2, whose couplings to the two respective right-handed neutrinos are controlled by an extra global U(1)N symmetry. We show that a flavon field is required to facilitate the effective Yukawa couplings, in order to implement the type I seesaw mechanism. We analyse the resulting phenomenology related to neutrino masses, flavour mixing and cosmological predictions concerning the formation and decay of topological defects like the global cosmic strings and the domain walls when the U(1)N × U(1)B−L symmetry is broken. The resulting gravitational wave spectrum is a distinctive combination of the spectrum from the global cosmic string and strong first-order phase transitions when the symmetries are broken, the strength of the latter being enhanced by the second Majoron field. The resulting characteristic spectrum determines the two right-handed neutrino mass scales within the considered framework.
hep-ph, astro-ph.CO
Fu, Bowen
e27ea734-314d-4092-8e7e-f6838017ab74
Ghoshal, Anish
61e009c4-becc-4864-a59d-e5a52820afe9
King, Stephen F.
f8c616b7-0336-4046-a943-700af83a1538
Fu, Bowen
e27ea734-314d-4092-8e7e-f6838017ab74
Ghoshal, Anish
61e009c4-becc-4864-a59d-e5a52820afe9
King, Stephen F.
f8c616b7-0336-4046-a943-700af83a1538
[Unknown type: UNSPECIFIED]
Abstract
In order to provide a natural framework for hierarchical right-handed neutrinos, we propose a realistic ultraviolet complete minimal multi-Majoron model (MMMM). We consider two right-handed neutrinos for simplicity, although the model is readily extendable to more. The minimal model introduces two complex scalar Majoron fields ϕ1 and ϕ2, whose couplings to the two respective right-handed neutrinos are controlled by an extra global U(1)N symmetry. We show that a flavon field is required to facilitate the effective Yukawa couplings, in order to implement the type I seesaw mechanism. We analyse the resulting phenomenology related to neutrino masses, flavour mixing and cosmological predictions concerning the formation and decay of topological defects like the global cosmic strings and the domain walls when the U(1)N × U(1)B−L symmetry is broken. The resulting gravitational wave spectrum is a distinctive combination of the spectrum from the global cosmic string and strong first-order phase transitions when the symmetries are broken, the strength of the latter being enhanced by the second Majoron field. The resulting characteristic spectrum determines the two right-handed neutrino mass scales within the considered framework.
Text
2507.08645v1
- Author's Original
Available under License Other.
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Accepted/In Press date: 11 July 2025
Additional Information:
19 pages, 4 figures
Keywords:
hep-ph, astro-ph.CO
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Local EPrints ID: 506700
URI: http://eprints.soton.ac.uk/id/eprint/506700
PURE UUID: 9ded837a-1579-4f97-b38b-d6111444b80e
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Date deposited: 14 Nov 2025 17:33
Last modified: 14 Nov 2025 17:33
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Author:
Bowen Fu
Author:
Anish Ghoshal
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