INFLATION AND AXION DARK MATTER IN THE 3-3-1 MODEL

Authors

  • Vu Hoa Binh Graduate University of Science and Technology, Vietnam Academy of Science and Technology,
  • Hoang Ngoc Long Graduate University of Science and Technology, Vietnam Academy of Science and Technology,
  • Vu Quang Tho Tan Trao Universty

DOI:

https://doi.org/10.51453/2354-1431/2022/877

Abstract

We consider a renormalizable theory, which successfully explains the number of Standard Model
(SM) fermion families and whose non-SM scalar sector includes an axion dark matter as well as
a field responsible for cosmological inflation. In such theory, the axion gets its mass via radiative
corrections at one-loop level mediated by virtual top quark, right handed Majorana neutrinos and
SM gauge bosons. Its mass is obtained in the range 4 keV÷ 40 keV, consistent with the one
predicted by XENON1T experiment, when the right handed Majorana neutrino mass is varied from
100 GeV up to 350 GeV, thus implying that the light active neutrino masses are generated from a low
scale type I seesaw mechanism. Furthermore, the theory under consideration can also successfully
accommodates the XENON1T excess provided that the PQ symmetry is spontaneously broken at
the 1010 GeV scale.
PACS numbers: 11.30.Fs, 12.15.Ff, 12.60.-i

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Published

2023-03-13

How to Cite

Vu Hoa, B., Hoang Ngoc, L., & Vu Quang, T. (2023). INFLATION AND AXION DARK MATTER IN THE 3-3-1 MODEL. SCIENTIFIC JOURNAL OF TAN TRAO UNIVERSITY, 9(1). https://doi.org/10.51453/2354-1431/2022/877

Issue

Vol. 9 No. 1 (2023): Special issue

Section

Natural Science and Technology

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