Mesonic stiff fluid distribution in five dimensional Bianchi type space time

DOI10.1007/s10509-007-9715-1zbMath1194.83074OpenAlexW2093485684MaRDI QIDQ931457

Elsie Sterbin Gottlieb

Publication date: 25 June 2008

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

Full work available at URL: https://doi.org/10.1007/s10509-007-9715-1

zbMATH Keywords

five dimensionsBianchi type space timesMesonic stiff fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Kaluza-Klein and other higher-dimensional theories (83E15)

Related Items (1)

ENERGY–MOMENTUM DISTRIBUTIONS OF FIVE-DIMENSIONAL HOMOGENEOUS-ANISOTROPIC UNIVERSES

Cites Work

• Bianchi type-II and III models in self-creation cosmology
• Bianchi \(type\)-VI\({}_ 0\) models in self-creation cosmology
• Radiating fluid distribution interacting with scalar field
• Inflationary universe: A possible solution to the horizon and flatness problems

This page was built for publication: Mesonic stiff fluid distribution in five dimensional Bianchi type space time