Bianchi type V barotropic perfect fluid cosmological model in Lyra geometry
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Publication:2390878
DOI10.1007/s10773-009-0002-5zbMath1171.83342OpenAlexW1973022572MaRDI QIDQ2390878
Publication date: 10 August 2009
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-009-0002-5
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (11)
A new class of Bianchi type-I cosmological models in Lyra geometry ⋮ Bulk viscous Bianchi type-V cosmological models with variable gravitational and cosmological constant ⋮ Bianchi type-III string cosmological model with bulk viscous fluid in Lyra geometry ⋮ Thick domain walls coupled with viscous fluid and electromagnetic field in Lyra geometry ⋮ New class of magnetized inhomogeneous Bianchi type-I cosmological model with variable magnetic permeability in Lyra geometry ⋮ A new class of inhomogeneous cosmological models with electromagnetic field in normal gauge for Lyra's manifold ⋮ Two-fluid cosmological model of Bianchi type-V with negative constant deceleration parameter ⋮ Anisotropic Bianchi type-III bulk viscous fluid universe in Lyra geometry ⋮ Invariant inhomogeneous Bianchi type-I cosmological models with electromagnetic fields using Lie group analysis in Lyra geometry ⋮ Bianchi type-III bulk viscous and barotropic perfect fluid cosmological models in Lyra's geometry ⋮ BIANCHI TYPE-I STRING DUST COSMOLOGICAL MODELS IN LYRA GEOMETRY
Cites Work
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