Bianchi type-III bulk-viscous string models in scalar-tensor theory of gravitation

DOI10.1142/S0219887824500208MaRDI QIDQ6489956

Y. Sobhanbabu, Y. Jnana Prasuna, Virinchi Srinivas, N. L. Pavan Kumar

Publication date: 22 April 2024

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

zbMATH Keywords

string cosmologybulk viscosityscalar-tensor theoryBianchi model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Anisotropic universe with cosmic strings and bulk viscosity in a scalar-tensor theory of gravitation
• Exact spatially homogeneous cosmologies
• Strong energy condition and the repulsive character of \(f(R)\) gravity
• The role of energy conditions in \(f(R)\) cosmology
• A new class of bulk viscous universe with time dependent deceleration parameter and \(\Lambda\)-term
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Holography Stabilizes the Vacuum Energy
• Isotropic homogeneous universe with viscous fluid
• Viscous Ricci dark energy and generalized second law of thermodynamics in modified f(R, T) gravity
• Cosmological parameters from SDSS and WMAP
• Dissipative cosmology
• The world as a hologram
• Viscous cosmology for early- and late-time universe
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Probable Values of the Cosmological Constant in a Holographic Theory

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