Some new Wyman–Leibovitz–Adler type static relativistic charged anisotropic fluid spheres compatible to self-bound stellar modeling

MH Murad, S Fatema - The European Physical Journal C, 2015 - Springer
In this work some families of relativistic anisotropic charged fluid spheres have been
obtained by solving the Einstein–Maxwell field equations with a preferred form of one of the …

Some static relativistic compact charged fluid spheres in general relativity

MH Murad, S Fatema - Astrophysics and Space Science, 2014 - Springer
In this work a new family of relativistic models of electrically charged compact star has been
obtained by solving Einstein–Maxwell field equations with preferred form of one of the metric …

Relativistic charged stellar modeling with a perfect fluid sphere

J Estevez-Delgado, JAR Ceballos… - Communications in …, 2023 - iopscience.iop.org
In this report we present the generalization of a solution to Einstein's equations with perfect
fluid for the case of Einstein–Maxwell with perfect fluid. The effect of the charge is reflected …

Closed form charged fluid with t = constant hypersurfaces as spheroids and hyperboloids

N Bijalwan, YK Gupta - Astrophysics and Space Science, 2012 - Springer
In the present article models of well behaved charged superdense stars with surface density
2× 10 14 gm/cm 3 are constructed by considering a static spherically symmetric metric with …

Some new Wyman-Adler type static relativistic charged anisotropic fluid spheres compatible to self-bound stellar modeling

MH Murad, S Fatema - arXiv preprint arXiv:1408.5126, 2014 - arxiv.org
In this work some families of relativistic anisotropic charged fluid spheres have been
obtained by solving Einstein-Maxwell field equations with preferred form of one of the metric …

[PDF][PDF] Some exact static charged perfect fluid spheres and relativistic compact Electrically charged stellar models in General Relativity

MH MURAD, S Fatema - Eur Phys JC, 2015 - researchgate.net
In this work some families of relativistic charged fluid spheres have been obtained by solving
Einstein-Maxwell field equations with preferred form of one of the metric potentials and a …

[PDF][PDF] A Family of Well Behaved Uncharged Model of Vaidya–Tikekar Type Super-Dense Star

J Kumar, AK Prasad - researchgate.net
In the present article a model of well-behaved uncharged superdense star with surface
density 2× 1014 gm/cm3 is developed by considering a static spherically symmetric metric …