Quadratically varying deceleration parameter in f(R,T) gravity

DOI10.1142/S0219887820300032MaRDI QIDQ6190544

Değer Sofuoğlu, Rishi Kumar Tiwari

Publication date: 5 March 2024

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

zbMATH Keywords

quintessencephantom\(f(R, T)\) theoryvarying deceleration parameter

Mathematics Subject Classification ID

Differential geometry (53-XX) Relativity and gravitational theory (83-XX)

Related Items (1)

Time varying deceleration parameter in \(f(R, T)\) gravity: a general case

Cites Work

• Cosmological models with linearly varying deceleration parameter
• Quantum de Sitter cosmology and phantom matter
• Cosmological perfect fluids in higher-order gravity
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Exact solutions of Bianchi type \(V\) spacetime in \(f(R,T)\) gravity
• A new type of isotropic cosmological models without singularity
• LRS Bianchi type-I cosmological model in \(f(R,T)\) theory of gravity
• Bianchi type-VI\({}_0\) perfect fluid cosmological model in a modified theory of gravity
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• The cosmological constant and dark energy
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Thermodynamics of dark energy
• Scenario of two-fluid dark energy models in Bianchi type-III Universe
• Cosmological perfect-fluids in f(R) gravity
• Cosmological model with variable deceleration parameter in f(R,T) modified gravity
• An alternative to quintessence

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