Bianchi type-VI\(_{h}\) string cloud cosmological models with bulk viscosity

DOI10.1007/s10509-010-0374-2zbMath1203.85019OpenAlexW2016512545MaRDI QIDQ613071

Dipanjali Behera, Sunil Kumar Tripathy

Publication date: 17 December 2010

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0374-2

zbMATH Keywords

bulk viscositystring clouddeceleration parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Stability and instability of geophysical and astrophysical flows (76E20) Astrophysical cosmology (85A40)

Related Items (2)

Energy and momentum of Bianchi type \(\mathrm{VI}_h\) universes ⋮ Some anisotropic universes in the presence of imperfect fluid coupling with spatial curvature

Cites Work

• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Massive string cloud cosmologies in Saez-Ballester theory of gravitation
• Some Bianchi type III string cosmological models with bulk viscosity
• Dissipative cosmology
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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