Cosmology with a master coupling in flipped SU(5)×U(1): The λ6 universe

Ellis, John; Garcia, Marcos A. G.; Nagata, Natsumi; Nanopoulos, Dimitri V.; Olive, Keith A.

doi:10.1016/j.physletb.2019.134864

Title: Cosmology with a master coupling in flipped SU(5)×U(1): The λ6 universe

Journal Article · 01 October 2019 · Physics Letters B

DOI: https://doi.org/10.1016/j.physletb.2019.134864 · OSTI ID:1564308

Ellis, John ^[1]; Garcia, Marcos A. G. ^[2]; Nagata, Natsumi ^[3]; Nanopoulos, Dimitri V. ^[4]; Olive, Keith A. ^[5]

King's College, London (United Kingdom). Dept. of Physics. Theoretical Particle Physics and Cosmology Group; European Organization for Nuclear Research (CERN), Geneva (Switzerland). Theoretical Physics Dept.; National Inst. of Chemical Physics and Biophysics, Tallinn (Estonia)
Rice Univ., Houston, TX (United States). Physics and Astronomy Dept.
Univ. of Tokyo (Japan). Dept. of Physics
Texas A & M Univ., College Station, TX (United States). George P. and Cynthia W. Mitchell Inst. for Fundamental Physics and Astronomy; Houston Advanced Research Center (HARC), Woodlands, TX (United States). Astroparticle Physics Group; Academy of Athens (Greece). Division of Natural Sciences
Univ. of Minnesota, Minneapolis, MN (United States). School of Physics and Astronomy. William I. Fine Theoretical Physics Inst.

We propose a complete cosmological scenario based on a flipped SU(5) × U(1) GUT model that incorporates Starobinsky-like inflation, taking the subsequent cosmological evolution carefully into account. A single master coupling, λ6, connects the singlet, GUT Higgs and matter fields, controlling 1) inflaton decays and reheating, 2) the gravitino production rate and therefore the non-thermal abundance of the supersymmetric cold dark matter particle, 3) neutrino masses and 4) the baryon asymmetry of the Universe.

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Research Organization:: Texas A & M Univ., College Station, TX (United States); Univ. of Minnesota, Minneapolis, MN (United States); Rice Univ., Houston, TX (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0010813; SC0011842; SC0018216; 17K14270; 18H05542; FG02-13ER42020

OSTI ID:: 1564308

Alternate ID(s):: OSTI ID: 1802182

Journal Information:: Physics Letters B, Vol. 797, Issue C; ISSN 0370-2693

Publisher:: ElsevierCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 18 works

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Inflation and leptogenesis in high-scale supersymmetry Kaneta, Kunio; Mambrini, Yann; Olive, Keith A. Physical Review D, Vol. 101, Issue 1 https://doi.org/10.1103/physrevd.101.015002	journal	January 2020
Inflation and Leptogenesis in High-Scale Supersymmetry Kaneta, Kunio; Mambrini, Yann; Olive, Keith A. arXiv https://doi.org/10.48550/arxiv.1911.02463	text	January 2019

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