Thermal stability of Tsallis holographic dark energy in nonflat universe

DOI10.1007/S10714-018-2497-7zbMath1409.83242OpenAlexW2908234099MaRDI QIDQ1710022

H. Moradpour, M. Abdollahi Zadeh, Ahmad Sheykhi

Publication date: 15 January 2019

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-018-2497-7

zbMATH Keywords

stabilityaccelerationTsallis entropydark energyholographic

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Quantum coherence, entanglement, quantum correlations (81P40) Astrophysical cosmology (85A40)

Related Items (8)

Effects of anisotropy on the sign-changeable interacting Tsallis holographic dark energy ⋮ Cosmic consequences of Barrow holographic dark energy with Granda-Oliveros cut-off in fractal cosmology ⋮ New Tsallis holographic dark energy with apparent horizon as IR-cutoff in non-flat Universe ⋮ Interacting Rényi holographic dark energy with parametrization on the interaction term ⋮ Phantom model for Tsallis holographic dark energy ⋮ Diagnosing the Sharma-Mittal holographic dark energy model through the statefinder ⋮ Thermodynamics and stability analysis of Tsallis holographic dark energy (THDE) models in \(F(\mathcal{R,T})\) gravity ⋮ Quintessence behavior of New Tsallis holographic dark energy in FRW universe

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