Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field

Details Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.143..377b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 143, no. 2, April 1988, p. 377-386.

Statistics

Computation

2

Astronomical Models, Computational Astrophysics, Cosmology, Electromagnetic Fields, Shear Flow, Viscous Fluids, Maxwell Equation, Relativistic Theory

Scientific paper

Some inhomogeneous viscous fluid cosmological models in the presence of an electromagnetic field for cylindrical symmetry are obtained. To get a determinate solution, it is assumed that the coefficient of shear viscosity is proportional to the rate of expansion. The paper also discusses the behaviour of the model when viscosity is absent and comments on some other physical properties.

Affiliated with

Also associated with

No associations

Rating

Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field 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 Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-847844