Bianchi Type I string dust cosmological model with magnetic field in general relativity

Details Bianchi Type I string dust cosmological model with magnetic field in general relativity Bianchi Type I string dust cosmological model with magnetic field in general relativity

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.312..305b&link_type=abstract

Astrophysics and Space Science, Volume 312, Issue 3-4, pp. 305-310

Mathematics

Logic

Bianchi I, String Dust, Magnetized, Cosmological

Scientific paper

Bianchi Type I string dust cosmological models in presence and absence of magnetic field following the techniques used by Letelier and Stachel, are investigated. To get the deterministic solution, we have assumed that σ {1/1} is proportional to the expansion ( θ) where σ {1/1} is the eigen value of shear tensor ( σ {/i j }) and which leads to A= N( BC)- n , n>0 where A, B, C are metric potentials and n=ell +1/3/ell -2/3 , N and ℓ are constants. The behaviour of the models in presence and absence of magnetic field are discussed. The other physical and geometrical aspects of the model are also discussed.

Affiliated with

Also associated with

No associations

Rating

Bianchi Type I string dust cosmological model with magnetic field in general relativity 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 Bianchi Type I string dust cosmological model with magnetic field in general relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bianchi Type I string dust cosmological model with magnetic field in general relativity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1526800