Energy conditions of the f(T, B) gravity dark energy model with the validity of thermodynamics

DOI10.1088/1572-9494/ab95fdzbMath1451.85012OpenAlexW3043896177MaRDI QIDQ5143563

S. H. Shekh, V. R. Chirde, P. K. Sahoo

Publication date: 12 January 2021

Published in: Communications in Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/1572-9494/ab95fd

zbMATH Keywords

thermodynamicsdark energyenergy conditions\(f(T,B)\) gravity

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items (5)

Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity ⋮ Observational constraints on teleparallel effective equation of state ⋮ f(T, B) gravity with statistically fitting of H(z) ⋮ A note on classification of locally rotationally symmetric Bianchi type I space–times via conformal vector fields in f(T,B) gravity ⋮ Observational constraints in accelerated emergent f(Q) gravity model

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