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

dc.contributor.authorHasegawa, Taiki
dc.contributor.authorOkada, Nobuchika
dc.contributor.authorSeto, Osamu
dc.contributor.otherHokkaido University
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.date.accessioned2022-08-02T15:11:59Z
dc.date.available2022-08-02T15:11:59Z
dc.date.issued2019
dc.description.abstractAn additional \(U\left(1\right)\) gauge interaction is one of the promising extensions of the standard model of particle physics. Among others, the \(U\left(1{\right)}_{B-L}\) 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 \(U\left(1{\right)}_{B-L}\) model, the symmetry breaking of the extra \(U\left(1\right)\) 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.en_US
dc.format.mimetypeapplication/pdf
dc.identifier.citationHasegawa, T., Okada, N., & Seto, O. (2019). Gravitational waves from the minimal gauged U(1)B−L model. In Physical Review D (Vol. 99, Issue 9). American Physical Society (APS). https://doi.org/10.1103/physrevd.99.095039
dc.identifier.doi10.1103/PhysRevD.99.095039
dc.identifier.urihttps://ir.ua.edu/handle/123456789/8761
dc.languageEnglish
dc.language.isoen_US
dc.publisherAmerican Physical Society
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subject1ST-ORDER PHASE-TRANSITION
dc.subjectB-L
dc.subjectRADIATION
dc.subjectVACUUM
dc.subjectSYMMETRY
dc.subjectAstronomy & Astrophysics
dc.subjectPhysics, Particles & Fields
dc.subjectPhysics
dc.titleGravitational waves from the minimal gauged U(1)(B-L) modelen_US
dc.typetext
dc.typeArticle

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