Bulk viscosity and decaying vacuum density in Friedmann universe
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Publication:1936383
DOI10.1007/s10773-012-1268-6zbMath1264.83058OpenAlexW2000849773MaRDI QIDQ1936383
Publication date: 4 February 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1268-6
Relativistic cosmology (83F05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (3)
Phase space analysis of bulk viscous matter dominated universe ⋮ Particle creation and bulk viscosity in Bianchi-I universe in Saez-Ballester theory with different deceleration parameters ⋮ LRS Bianchi type II massive string cosmological model for stiff fluid distribution with decaying vacuum energy \((\varLambda)\)
Cites Work
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- The cosmological constant is back
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- Friedmann cosmology with decaying vacuum density
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- BIANCHI TYPE I UNIVERSE WITH VISCOUS FLUID
- The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid
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