Scalar field and time varying cosmological constant in \(f(R, T)\) gravity for Bianchi type-I universe

DOI10.1016/J.CJPH.2016.04.010arXiv1506.08055OpenAlexW3103993005MaRDI QIDQ6199349

P. K. Sahoo, G. P. Singh, Binaya K. Bishi

Publication date: 23 February 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1506.08055

zbMATH Keywords

cosmological constantscalar field\(f(R, T)\) gravityLRS Bianchi type-I spacetime

Mathematics Subject Classification ID

Local differential geometry (53Bxx) Differential geometry (53-XX) Relativistic cosmology (83Fxx)

Related Items (2)

Whether Lyra's manifold itself is a hidden source of dark energy ⋮ Scalar field cosmology in \(f(R,T)\) gravity with \(\Lambda\)

Cites Work

• Nonlinear gravitational Lagrangians
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Anisotropic cosmological models with quintessence
• FRW MODELS WITH PERFECT FLUID AND SCALAR FIELD IN HIGHER DERIVATIVE THEORY
• <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
• Exact scalar field cosmologies
• Scalar field cosmologies with barotropic matter: models of Bianchi class B
• Tachyon field as a dark energy in Bianchi type-V spacetime
• Inflationary universe: A possible solution to the horizon and flatness problems
• Cosmological Imprint of an Energy Component with General Equation of State
• General Relativity

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