Self-anisotropizing inflationary universe in Horndeski theory and beyond

DOI10.1088/1475-7516/2018/07/058OpenAlexW3105588028WikidataQ129486039 ScholiaQ129486039MaRDI QIDQ5023081

Tsutomu Kobayashi, Sakine Nishi, Hiroaki W. H. Tahara, Jun'ichi Yokoyama

Publication date: 20 January 2022

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

Full work available at URL: https://arxiv.org/abs/1805.00186

zbMATH Keywords

inflationmodified gravityphysics of the early universe

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (4)

From matter to galaxies: general relativistic bias for the one-loop bispectrum ⋮ Effective field theory of anisotropic inflation and beyond ⋮ Imprints of Schwinger effect on primordial spectra ⋮ Anisotropic inflation with coupled p−forms

Cites Work

• A new type of isotropic cosmological models without singularity
• Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
• Inflationary cosmology: First 30+ years
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• Inflationary universe: A possible solution to the horizon and flatness problems

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