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Cosmological Models with Big Rip and Pseudo Rip Scenarios in Extended Theory of Gravity

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Publication:6066528
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DOI10.1002/prop.202100086arXiv2107.04413OpenAlexW3200639862MaRDI QIDQ6066528

Sunil Kumar Tripathy, Sankarsan Tarai, Pratik P. Ray, B. Mishra

Publication date: 16 November 2023

Published in: Fortschritte der Physik (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2107.04413


zbMATH Keywords

perfect fluidbig ripextended gravitypseudo rip


Mathematics Subject Classification ID

Quantum theory (81-XX)


Related Items

The fate of the universe evolution in the quadratic form of Ricci-Gauss-Bonnet cosmology ⋮ Oscillating gravity, non-singularity and mass quantization from Moffat stochastic gravity arguments



Cites Work

  • The phantom divide in string gas cosmology
  • Quantum de Sitter cosmology and phantom matter
  • Energy and momentum of Bianchi type \(\mathrm{VI}_h\) universes
  • From Big to Little Rip in modified \(F(R,G)\) gravity
  • Exorcising \(w < -1\)
  • Cosmological models with a hybrid scale factor in an extended gravity theory
  • Sudden future singularities
  • BIG RIP AND LITTLE RIP SOLUTIONS IN SCALAR MODEL WITH KINETIC AND GAUSS–BONNET COUPLINGS
  • Cosmological evolution, future singularities, Little Rip and Pseudo-Rip in viable f(R) theories and their scalar–tensor counterpart
  • Future state of the universe
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