• Open Access

SU(5)×U(1)X axion model with observable proton decay

Nobuchika Okada, Digesh Raut, and Qaisar Shafi
Phys. Rev. D 104, 055041 – Published 27 September 2021

Abstract

We propose a SU(5)×U(1)X×U(1)PQ model, where U(1)X is the generalization of the BL (baryon minus lepton number) gauge symmetry and U(1)PQ is the global Peccei-Quinn (PQ) symmetry. There are four fermions families in 5¯+10 representations of SU(5), a mirror family in 5+10¯ representations, and three SU(5) singlet Majorana fermions. The U(1)X related anomalies all cancel in the presence of the Majorana neutrinos. The SU(5) symmetry is broken at MGUT(69)×1015GeV and the proton lifetime τp is estimated to be well within the expected sensitivity of the future hyper-Kamiokande experiment, τp1.3×1035years. The SU(5) breaking also triggers the breaking of the PQ symmetry, resulting in axion dark matter (DM), with the axion decay constant fa of order MGUT or somewhat larger. The CASPEr experiment can search for such an axion DM candidate. The Hubble parameter during inflation must be low, Hinf109GeV, in order to successfully resolve the axion domain wall, axion DM isocurvature and SU(5) monopole problems. With the identification of the U(1)X breaking Higgs field with the inflaton field, we implement inflection-point inflation, which is capable of realizing the desired value for Hinf. The vectorlike fermions in the model are essential for achieving successful unification of the SM gauge couplings as well as the phenomenological viability of both axion DM and inflation scenario.

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  • Received 8 July 2021
  • Accepted 9 August 2021

DOI:https://doi.org/10.1103/PhysRevD.104.055041

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Nobuchika Okada1,*, Digesh Raut2,†, and Qaisar Shafi2,‡

  • 1Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487, USA
  • 2Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA

  • *okadan@ua.edu
  • draut@udel.edu
  • qshafi@udel.edu

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Issue

Vol. 104, Iss. 5 — 1 September 2021

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