Cylindrically symmetric inhomogeneous cosmological models with viscous fluid and varying \(\Lambda\)

DOI10.1007/s10582-006-0125-3zbMath1105.83022OpenAlexW2021948977MaRDI QIDQ2508665

Anirudh Pradhan, Prashant Singh, Kanti Jotania

Publication date: 20 October 2006

Published in: Czechoslovak Journal of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10582-006-0125-3

zbMATH Keywords

cosmologyvariable cosmological constantinhomogeneous models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (9)

Cylindrically symmetric relativistic fluids and the purely electric Weyl tensor ⋮ The signature of string ball near surface horizon of cylindrical universe ⋮ A new class of inhomogeneous cosmological models with electromagnetic field in normal gauge for Lyra's manifold ⋮ Higher dimensional FRW cosmology with variable G and \(\Lambda \) ⋮ Plane symmetric viscous fluid cosmological models with varying \(\Lambda\)-term ⋮ Accelerated Lyra's cosmology driven by electromagnetic field in inhomogeneous universe ⋮ A new class of relativistic perfect fluid cylinders with expansion proportional to shear scalar ⋮ Unnamed Item ⋮ Cylindrically symmetric inhomogeneous universes with a cloud of strings

Cites Work

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• Dissipative cosmology
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• Cosmic strings and domain walls
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