Smooth μ-hybrid and non-minimal Higgs inflation in SU(4) <sub>C</sub> × SU(2)<sub> L </sub> × SU(2)<sub> R </sub> with observable gravitational waves

Abstract We propose to study a smooth variant of the μ -hybrid inflation model and a non-minimal Higgs model of inflation with quartic non-minimal coupling between the Higgs field and gravity within the context of a realistic GUT gauge group based on supersymmetric SU(4) C × SU(2) L × SU(2) R . These models are incorporated with a realistic scenario of reheating and non-thermal leptogenesis, compatible with the constraints from the baryon asymmetry of the universe. Notably, both models successfully address the MSSM μ -problem and avoid the issue of primordial magnetic monopoles. Our analysis reveals that both models predict a scalar spectral index n s that closely aligns with the central observationally favored value of Planck2018 + BICEP2/Keck Array (BK15) data and yield a large tensor-to-scalar ratio ( r &gt; 10 -3 ), potentially detectable in forthcoming CMB experiments.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-02-01
DOI
https://doi.org/10.1088/1475-7516/2025/02/033
Citations
3
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
3.46
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article

Smooth μ-hybrid and non-minimal Higgs inflation in SU(4) C × SU(2) L × SU(2) R with observable gravitational waves

Umer Zubair
3 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
3.46
article

Smooth μ-hybrid and non-minimal Higgs inflation in SU(4) C × SU(2) L × SU(2) R with observable gravitational waves

Umer Zubair
article en
3 citations

Abstract

Abstract We propose to study a smooth variant of the μ -hybrid inflation model and a non-minimal Higgs model of inflation with quartic non-minimal coupling between the Higgs field and gravity within the context of a realistic GUT gauge group based on supersymmetric SU(4) C × SU(2) L × SU(2) R . These models are incorporated with a realistic scenario of reheating and non-thermal leptogenesis, compatible with the constraints from the baryon asymmetry of the universe. Notably, both models successfully address the MSSM μ -problem and avoid the issue of primordial magnetic monopoles. Our analysis reveals that both models predict a scalar spectral index n s that closely aligns with the central observationally favored value of Planck2018 + BICEP2/Keck Array (BK15) data and yield a large tensor-to-scalar ratio ( r &gt; 10 -3 ), potentially detectable in forthcoming CMB experiments.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(02)
University of Delaware (US)
Openalex Percentile: Top 9%
Cosmology and Gravitation Theories
3.46
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Smooth μ-hybrid and non-minimal Higgs inflation in SU(4) <sub>C</sub> × SU(2)<sub> L </sub> × SU(2)<sub> R </sub> with observable gravitational waves — Umer Zubair · Journal of Cosmology and Astroparticle Physics (2025) | TGRS Research Map | TGRS