Bouncing cosmological isotropic solutions in scalar-tensor gravity
DOI10.1088/1475-7516/2022/01/052zbMath1486.83035arXiv2111.07319OpenAlexW3211993712MaRDI QIDQ5863317
David Polarski, Y. Verbin, Alexei A. Starobinsky
Publication date: 11 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2111.07319
Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Groups and algebras in quantum theory and relations with integrable systems (81R12) Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Matrix models and tensor models for quantum field theory (81T32)
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Cites Work
- Dynamical study of the singularities of gravity in the presence of nonminimally coupled scalar fields
- Bouncing cosmologies: progress and problems
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Cosmology or Catastrophe? A non-minimally coupled scalar in an inhomogeneous universe
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- A nonsingular universe
- Simplest Cosmological Model with the Scalar Field
- SIMPLEST COSMOLOGICAL MODEL WITH THE SCALAR FIELD II.
- A classical, non-singular, bouncing universe
- Interdependence between integrable cosmological models with minimal and non-minimal coupling