Gravitational waves from the minimal gauged U(1)B–L model

Hasegawa, Taiki; Okada, Nobuchika; Seto, Osamu

doi:10.1103/physrevd.99.095039

Title: Gravitational waves from the minimal gauged U(1)_B–L model

Journal Article · 28 May 2019 · Physical Review D

DOI: https://doi.org/10.1103/physrevd.99.095039 · OSTI ID:1518503

Hasegawa, Taiki ^[1]; Okada, Nobuchika ^[2]; Seto, Osamu ^[1]

Hokkaido Univ., Sapporo (Japan)
Univ. of Alabama, Tuscaloosa, AL (United States)

An additional U(1) gauge interaction is one of the promising extensions of the standard model of particle physics. Among others, the U(1)_B–L gauge symmetry is particularly interesting because it addresses the origin of Majorana masses of right-handed neutrinos, which naturally leads to tiny light neutrino masses through the seesaw mechanism. We show that, based on the minimal U(1)_B–L model, the symmetry breaking of the extra U(1) gauge symmetry with its minimal Higgs sector in the early universe can exhibit the first-order phase transition and hence generate a large enough amplitude of stochastic gravitational wave radiation that is detectable in future experiments.

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Research Organization:: Univ. of Alabama, Tuscaloosa, AL (United States)

Sponsoring Organization:: USDOE Office of Science (SC); USDOE

Grant/Contract Number:: SC0012447; 19K03860; 19H05091

OSTI ID:: 1518503

Alternate ID(s):: OSTI ID: 1611811

Journal Information:: Physical Review D, Vol. 99, Issue 9; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Title: Gravitational waves from the minimal gauged U(1)_B–L model