Marder space-time with Tsallis holographic dark energy

DOI10.1142/S0219887822502115zbMath1530.83011WikidataQ114072243 ScholiaQ114072243MaRDI QIDQ6191591

T. Chinnappalanaidu, M. Vijaya Santhi

Publication date: 9 February 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

cosmologydark energy modelTsallis holographic dark energyMarder-type space-time

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15) Dark matter and dark energy (83C56)

Cites Work

• Dark energy models in \(f(R,T)\) theory with variable deceleration parameter
• Anisotropic viscous fluid cosmological models from deceleration to acceleration in string cosmology
• Dark energy models with anisotropic fluid in Bianchi type-\(VI _{0}\) space-time with time dependent deceleration parameter
• Cosmological models with linearly varying deceleration parameter
• Non-existence of a massive scalar field for the Marder universe in Lyra and Riemannian geometries
• Bianchi type-V bulk viscous cosmic string in \(f(R, T)\) gravity with time varying deceleration parameter
• Bianchi type-I space-time with variable cosmological constant
• Exact spatially homogeneous cosmologies
• Gravitational waves in general relativity I. Cylindrical waves
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Relationship between magnetic field and anisotropy parameter in gravitation theories
• Bulk viscous Bianchi-I embedded cosmological model in f(R,T) = f1(R) + f2(R)f3(T) gravity
• Various dark energy models with time-varying G and Λ in f(R, T) gravitation theory
• Cosmic jerk, snap and beyond
• The cosmological constant problem
• Einstein's General Theory of Relativity
• An alternative to quintessence

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