Plane-symmetric mesonic viscous fluid cosmological model

DOI10.1007/BF00645149zbMath0890.76099MaRDI QIDQ1368940

Bernhard Rupp

Publication date: 7 October 1997

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

zbMATH Keywords

Einstein field equationsattractive scalar fieldsnonstatic solutionsstrong interaction of elementary particles

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (12)

SOME BIANCHI TYPE COSMOLOGICAL MODELS IN LYRA GEOMETRY ⋮ Spatially homogeneous Bianchi type-I universes with variable \(G\) and \(\Lambda \) ⋮ Bianchi types II, VIII and IX string cosmological models with bulk viscosity in Brans-Dicke theory of gravitation ⋮ LRS Bianchi type-II universe with cosmic strings and bulk viscosity in a scalar tensor theory of gravitation ⋮ Bianchi types II, VIII, and IX string cosmological models with bulk viscosity in a theory of gravitation ⋮ Kaluza-Klein universe with cosmic strings and bulk viscosity in a scalar-tensor theory of gravitation ⋮ Anisotropic universe with cosmic strings and bulk viscosity in a scalar-tensor theory of gravitation ⋮ Massive and massless scalar field models for Kaluza–Klein universe in f(R, T) gravity ⋮ Modified Chaplygin gas cosmology with bulk viscosity ⋮ Scalar field cosmology in \(f(R,T)\) gravity with \(\Lambda\) ⋮ Bianchi type-III cosmological models in Lyra's geometry in the presence of massive scalar field ⋮ Dynamical Anisotropic Dark Energy Cosmological Model in General Relativity

Cites Work

• Cosmological mesonic viscous fluid model
• Reformulation of general relativity in accordance with Mach's principle
• Relativity theory and the creation of matter
• Empty space-times admitting a three parameter group of motions

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