A new family of polynomial solutions for charged fluid spheres
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Publication:420098
DOI10.1016/J.NONRWA.2011.08.008zbMath1238.35158OpenAlexW1965962416MaRDI QIDQ420098
Y. K. Gupta, Sunil Kumar Maurya
Publication date: 20 May 2012
Published in: Nonlinear Analysis. Real World Applications (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/j.nonrwa.2011.08.008
PDEs in connection with relativity and gravitational theory (35Q75) Solutions to PDEs in closed form (35C05) Einstein-Maxwell equations (83C22)
Related Items (6)
Determination of the charge for strange stars ⋮ Charged fluid to anisotropic fluid distribution in general relativity ⋮ Well behaved charged generalization of Buchdahl's fluid spheres ⋮ Some exact relativistic models of electrically charged self-bound stars ⋮ Exact well behaved solutions of Einstein-Maxwell equations for relativistic charged superdense star models ⋮ A study on charged compact stars
Cites Work
- A family of physically realizable perfect fluid spheres representing a \(quark\)-\(stars\) in general relativity
- New class of regular and well behaved exact solutions in general relativity
- Extremization of mass of charged superdense star models describe by Durgapal type space-time metric
- New class of well behaved exact solutions of relativistic charged white-dwarf star with perfect fluid
- Equilibrium of a static charged perfect fluid sphere
- Some new static charged spheres
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Some new exact solutions with finite central parameters and uniform radial motion of sound
- Generating potentials via difference equations
- Tikekar superdense stars in electric fields
- Exact models for isotropic matter
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