Mathematical Research Data Initiative
Main page
Recent changes
Random page
Help about MediaWiki
Create a new Item
Create a new Property
Create a new EntitySchema
Merge two items
In other projects
Discussion
View source
View history
Purge
English
Log in

Cosmological viscous fluid models in the presence of electromagnetic field and zero-mass scalar field

From MaRDI portal
Publication:1115322
Jump to:navigation, search

DOI10.1007/BF00641726zbMath0663.76153OpenAlexW2059081481MaRDI QIDQ1115322

S. H. Smith

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1007/bf00641726


zbMATH Keywords

electromagnetic fieldviscous fluidzero-mass scalar fieldimperfect fluid FRW modelsspherically-symmetric Robertson-Walker metric


Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)


Related Items

Non-existence of a massive scalar field for the Marder universe in Lyra and Riemannian geometries ⋮ The decay of massive scalar field in non-static Gödel type universe with viscous fluid and heat flow ⋮ Viscous inflationary universe models



Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:1115322&oldid=13160077"
Tools
What links here
Related changes
Special pages
Printable version
Permanent link
Page information
MaRDI portal item
This page was last edited on 31 January 2024, at 03:37.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki