Magneto-viscous fluid cosmological models in presence of zero-mass scalar field

Details Magneto-viscous fluid cosmological models in presence of zero-mass scalar field Magneto-viscous fluid cosmological models in presence of zero-mass scalar field

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205..277r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 2, p. 277-282.

Statistics

Computation

3

Astronomical Models, Electromagnetic Fields, Interstellar Magnetic Fields, Viscous Fluids, Computational Astrophysics, Scalars

Scientific paper

A viscous fluid cosmological model in presence of magnetic field and
zero-mass scalar fields is developed. The non-negativity condition of
viscous fluid pressure prescribes a certain minimum value of t vis-a-vis
the scale factor Q(t), and at this epoch the model is found to be
singularity-free.

Affiliated with

Also associated with

No associations

Rating

Magneto-viscous fluid cosmological models in presence of zero-mass scalar 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 Magneto-viscous fluid cosmological models in presence of zero-mass scalar field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magneto-viscous fluid cosmological models in presence of zero-mass scalar field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1068473