Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.332..403p&link_type=abstract
Astrophysics and Space Science, Volume 332, Issue 2, pp.403-408
Astronomy and Astrophysics
Astrophysics
6
Charge Fluid, Reissner-Nordstrom, General Relativity, Exact Solution
Scientific paper
The paper presents a class of interior solutions of Einstein-Maxwell field equations of general relativity for a static, spherically symmetric distribution of the charged fluid. This class of solutions describes well behaved charged fluid balls. The class of solutions gives us wide range of parameter K (0≤ K≤42) for which the solution is well behaved hence, suitable for modeling of super dense star. For this solution the mass of a star is maximized with all degree of suitability and by assuming the surface density ρ b =2×1014 g/cm3. Corresponding to K=2 and X=0.30, the maximum mass of the star comes out to be 4.96 M Θ with linear dimension 34.16 km and central redshift and surface redshift 2.1033 and 0.683 respectively. In absence of the charge we are left behind with the well behaved fourth model of Durgapal (J. Phys., A, Math. Gen. 15:2637, 1982).
No associations
LandOfFree
Well behaved parametric class of relativistic charged fluid ball 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 Well behaved parametric class of relativistic charged fluid ball in general relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Well behaved parametric class of relativistic charged fluid ball in general relativity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1183882