Deprecated: $wgMWOAuthSharedUserIDs=false is deprecated, set $wgMWOAuthSharedUserIDs=true, $wgMWOAuthSharedUserSource='local' instead [Called from MediaWiki\HookContainer\HookContainer::run in /var/www/html/w/includes/HookContainer/HookContainer.php at line 135] in /var/www/html/w/includes/Debug/MWDebug.php on line 372
Bianchi type-I cosmological model for perfect fluid distribution in Lyra geometry - MaRDI portal

Bianchi type-I cosmological model for perfect fluid distribution in Lyra geometry

From MaRDI portal
Publication:3544661

DOI10.1063/1.2898477zbMath1153.85310OpenAlexW2004722917MaRDI QIDQ3544661

Naresh K. Chandnani, Raj Bali

Publication date: 8 December 2008

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

Full work available at URL: https://doi.org/10.1063/1.2898477




Related Items (20)

A new class of Bianchi type-I cosmological models in Lyra geometryBianchi type-III cosmological models with time dependent displacement vector for barotropic fluid distribution in Lyra geometryA plane-symmetric magnetized inhomogeneous cosmological models of perfect fluid distribution with variable magnetic permeability in Lyra geometryBianchi type V barotropic perfect fluid cosmological model in Lyra geometryBianchi type-III string cosmological model with bulk viscous fluid in Lyra geometryNew class of magnetized inhomogeneous Bianchi type-I cosmological model with variable magnetic permeability in Lyra geometrySpatially homogeneous Bianchi type IX dust filled universe with time dependent displacement vector in Lyra geometryBianchi type I magnetized stiff fluid models with bulk viscosity in Lyra geometryAnisotropic Bianchi type-I string cosmological models in normal gauge for Lyra's manifold with constant deceleration parameterA new class of inhomogeneous cosmological models with electromagnetic field in normal gauge for Lyra's manifoldLRS Bianchi type II perfect fluid cosmological models in normal gauge for Lyra's manifoldInvariant inhomogeneous Bianchi type-I cosmological models with electromagnetic fields using Lie group analysis in Lyra geometryLRS Bianchi type II massive string cosmological models with magnetic field in Lyra's geometryAccelerated Lyra's cosmology driven by electromagnetic field in inhomogeneous universeBianchi type-III bulk viscous and barotropic perfect fluid cosmological models in Lyra's geometryBIANCHI TYPE-I STRING DUST COSMOLOGICAL MODELS IN LYRA GEOMETRYBIANCHI TYPE I MAGNETIZED DUST FILLED UNIVERSE IN LYRA GEOMETRYBianchi type-I string dust models with bulk viscosity in Lyra geometryBianchi type-IX barotropic fluid model with time-dependent displacement vector in Lyra geometryCylindrically symmetric viscous fluid universe in Lyra geometry




Cites Work




This page was built for publication: Bianchi type-I cosmological model for perfect fluid distribution in Lyra geometry