Massive scalar field interacting with viscous fluid distribution in cosmological models

Details Massive scalar field interacting with viscous fluid distribution in cosmological models Massive scalar field interacting with viscous fluid distribution in cosmological models

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.150...65t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 150, no. 1, Dec. 1988, p. 65-74.

Physics

2

Astronomical Models, Cosmology, Field Theory (Physics), Viscous Fluids, Cosmic Dust, Hubble Constant, Klein-Gordon Equation, Partial Differential Equations, Scalars

Scientific paper

The study of Einstein's field equations describing Robertson-Walker cosmological models with massive scalar field and viscous fluid representing the matter has been made. The problem has been investigated with and without the source density in the wave equation. Corresponding exact solutions of the field equations have been obtained under different physical equations of state, including dust distribution, Zeldovich fluid distribution, disordered distribution of radiation subject to physically realistic conditions. It has been found that physically realistic solutions have been obtained for closed cosmological models only.

Affiliated with

Also associated with

No associations

Rating

Massive scalar field interacting with viscous fluid distribution in cosmological models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Massive scalar field interacting with viscous fluid distribution in cosmological models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Massive scalar field interacting with viscous fluid distribution in cosmological models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1752758