Tsallis holographic dark energy model with event horizon cutoff in modified gravity
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Publication:6541432
DOI10.1142/S0219887822502346zbMATH Open1543.83171MaRDI QIDQ6541432
Alexander S. Tepliakov, Artyom V. Astashenok
Publication date: 17 May 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)
Cites Work
- Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories
- Particle creation by black holes
- Beyond Einstein gravity. A survey of gravitational theories for cosmology and astrophysics.
- Non-perturbative 2 particle scattering amplitudes in \(2+1\) dimensional quantum gravity
- Cosmological constant -- the weight of the vacuum
- Possible generalization of Boltzmann-Gibbs statistics.
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Holographic dark energy
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- The cosmological constant and dark energy
- DYNAMICS OF DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Extensions of f(R) Gravity
- Cosmological implications of Tsallis dark energy in modified Brans–Dicke theory
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Black Holes and Entropy
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