Interacting anisotropic ghost dark energy model in \(f(R,T)\) theory of gravity

DOI10.1134/S0202289321010072zbMath1480.83064OpenAlexW3138559414MaRDI QIDQ2054888

Kanika Das, Jumi Bharali

Publication date: 3 December 2021

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289321010072

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)

Cites Work

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• The QCD nature of dark energy
• Cosmological evolution of quintessence and phantom with a new type of interaction in dark sector
• Le Châtelier-Braun principle in cosmological physics
• Kaluza-Klein cosmological model in \(f(R,T)\) gravity
• Bianchi type-III dark energy model in \(f(R,T)\) gravity
• Bianchi type-III cosmological model in \(f(R,T)\) theory of gravity
• Holographic dark energy (DE) cosmological models with quintessence in Bianchi type-V space time
• LRS Bianchi type-I cosmological model in \(f(R,T)\) theory of gravity
• Cosmography: Cosmology without the Einstein equations
• Cosmological Constraints on the Sign-Changeable Interactions
• The cosmological constant and dark energy
• Mach's Principle and a Relativistic Theory of Gravitation
• Cosmological parameters from SDSS and WMAP
• Jerk, snap and the cosmological equation of state
• Phantom fluid supporting traversable wormholes in alternative gravity with extra material terms
• The cosmological constant problem

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