Radiation-like imperfect fluid cosmologies

Details Radiation-like imperfect fluid cosmologies Radiation-like imperfect fluid cosmologies

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...288..418c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 288, Jan. 15, 1985, p. 418-421.

Statistics

Computation

27

Computational Astrophysics, Cosmology, Einstein Equations, Extraterrestrial Radiation, Viscous Fluids, Astronomical Models, Field Theory (Physics), Magnetohydrodynamics

Scientific paper

Radiation-like viscous fluid solutions of the Einstein field equations are presented in which the geometrical part corresponds to the k = 0, R(t) = t exp 1/2 FRW model. It is shown that there are radial solutions, in particular, self-similar solutions, corresponding to the spacetime and which describe radiating imperfect fluids, that are valid everywhere and satisfy all necessary physical requirements. Such solutions are of importance in hydrodynamics, including viscous fluid motion, in astrophysics, and in cosmology.

Affiliated with

Also associated with

No associations

Rating

Radiation-like imperfect fluid cosmologies 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 Radiation-like imperfect fluid cosmologies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation-like imperfect fluid cosmologies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-925307