Multi-chaotic inflation with and without spectator field

DOI10.1088/1475-7516/2022/07/042OpenAlexW4226242991MaRDI QIDQ5101102

Tomo Takahashi, Shuichiro Yokoyama, Yukiyoshi Morishita

Publication date: 2 September 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2203.09698

zbMATH Keywords

inflationphysics of the early universeinflation and CMBR theory

Mathematics Subject Classification ID

Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Quantum optics (81V80) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (1)

Cosmic acceleration in Lovelock quantum gravity

Cites Work

• Leptogenesis after chaotic sneutrino inflation and the supersymmetry breaking scale
• Sneutrino driven GUT inflation in supergravity
• Superconformal inflationary \(\alpha\)-attractors
• Chaotic inflation with right-handed sneutrinos after Planck
• Supergravity-based inflation models: a review
• A general proof of the conservation of the curvature perturbation
• Effects of cosmological moduli fields on cosmic microwave background
• Generating the curvature perturbation without an inflaton

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