Non-flat FRW universe version of Tsallis holographic dark energy in specific modified gravity
DOI10.1142/S021773231950055XzbMath1409.83153OpenAlexW2920713332MaRDI QIDQ4629308
Nadeem Azhar, Abdul Jawad, Shamaila Rani
Publication date: 21 March 2019
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s021773231950055x
stabilitygeneralized second law of thermodynamicscosmological parametersdynamical Chern-Simons modify gravityTsallis holographic dark energy model
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)
Cites Work
- Generalized second law of thermodynamics in \(f(T)\) gravity with entropy corrections
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- de Sitter brane universe induced by phantom and quantum effects
- Quantum de Sitter cosmology and phantom matter
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- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- DYNAMICS OF DARK ENERGY
- Cosmological implications of dark energy models in modified gravity
- The cosmological constant problem
- Thermodynamic properties of modified gravity theories
- \(k\)-inflation
- An alternative to quintessence
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