Some exact relativistic models of electrically charged self-bound stars
DOI10.1007/S10773-013-1752-7zbMath1282.83011OpenAlexW2070854247MaRDI QIDQ2436472
Mohammad Hassan Murad, Saba Fatema
Publication date: 25 February 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1752-7
exact solutiongeneral relativityastrophysicsequation of statecompact starscharged fluid sphereReissner-Nordströmrelativistic starsEinstein-MaxwellSchwarzschild coordinatesself-bound stars
Black holes (83C57) Strong interaction, including quantum chromodynamics (81V05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)
Related Items (3)
Cites Work
- An exact family of Einstein-Maxwell Wyman-Adler solution in general relativity
- A relativistic model for strange quark star
- Well behaved parametric class of relativistic charged fluid ball in general relativity
- Well behaved class of charge analogue of heintzmann's relativistic exact solution
- On a family of well behaved perfect fluid balls as astrophysical objects in general relativity
- A new family of polynomial solutions for charged fluid spheres
- New class of well behaved exact solutions for static charged neutron-star with \textit{perfect fluid}
- A class of charged relativistic superdense star models
- Relativistic modeling of charged super-dense star with Einstein-Maxwell equations in general relativity
- A class of regular and well behaved relativistic super-dense star models
- Variety of well behaved parametric classes of relativistic charged fluid spheres 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
- Sharp bounds on the critical stability radius for relativistic charged spheres
- Minimum mass-radius ratio for charged gravitational objects
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Exact interior solutions for charged fluid spheres
- Relativistic modelling of a superdense star containing a charged perfect fluid
- Some new exact solutions with finite central parameters and uniform radial motion of sound
- A family of charge analogue of Durgapal solution
- Well-behaved relativistic charged super-dense star models
- A family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativity
- A well-behaved class of charged analogue of Durgapal solution
- A new well behaved class of charge analogue of Adler's relativistic exact solution
- RELATIVISTIC SOLUTION FOR A CLASS OF STATIC COMPACT CHARGED STAR IN PSEUDO-SPHEROIDAL SPACETIME
- Tikekar superdense stars in electric fields
- ANALYTICAL MODELS FOR QUARK STARS
- Singularity-free static fluid spheres in general relativity
- REGULAR AND WELL-BEHAVED RELATIVISTIC CHARGED SUPERDENSE STAR MODELS
- MAXIMUM MASS OF A CLASS OF COLD COMPACT STARS
- QUARK STARS ADMITTING A ONE-PARAMETER GROUP OF CONFORMAL MOTIONS
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- Radially Symmetric Distributions of Matter
- General solution for a class of static charged spheres
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