Radiating fluid distribution interacting with scalar field

DOI10.1007/BF00668899zbMath0663.76155OpenAlexW1981102074MaRDI QIDQ1115323

Koijam Manihar Singh

Publication date: 1988

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00668899

zbMATH Keywords

energy-momentum tensorperfect fluidzero-mass scalar fieldspherically symmetric Einstein universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (4)

Radiating viscous universes coupled with zero-mass scalar field: Exact solutions ⋮ Mesonic stiff fluid distribution in five dimensional Bianchi type space time ⋮ Rotational perturbations of radiating universes coupled with zero-mass scalar field ⋮ The decay of massive scalar field in non-static Gödel type universe with viscous fluid and heat flow

Cites Work

• Viscous fluid universe interacting with scalar field
• A class of exact solutions of certain classical field equations in general relativity
• Conformally flat static space–time in Brans–Dicke theory
• A new basis for cosmology
• Nonstatic Solutions of Einstein's Field Equations for Spheres of Fluids Radiating Energy
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