On the expanding phase of a singular bounce and intermediate inflation: The modified gravity description
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Publication:2985017
DOI10.1142/S0217732317500675zbMath1360.83058arXiv1703.06713OpenAlexW2599694180MaRDI QIDQ2985017
Publication date: 15 May 2017
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1703.06713
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)
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Modified gravity theories on a nutshell: inflation, bounce and late-time evolution ⋮ Cosmic acceleration and ekpyrotic bounce with Chameleon field ⋮ Loop quantum cosmology-corrected Gauss–Bonnet singular cosmology ⋮ Holographic dark energy models in higher derivative torsion corrected modified teleparallel gravity
Cites Work
- Warm intermediate inflation in \(F(T)\) gravity
- Constraints on singular evolution from gravitational baryogenesis
- Singular F ( R ) cosmology unifying early- and late-time acceleration with matter and radiation domination era
- Matter bounce cosmology with the f ( T ) gravity
- More general sudden singularities
- Sudden future singularities in FLRW cosmologies
- New isotropic and anisotropic sudden singularities
- Intermediate inflation and the slow-roll approximation
- Sudden future singularities
- General dissipative coefficient in warm intermediate inflation in Loop Quantum Cosmology in light of Planck and BICEP2