Relativistic modeling of charged super-dense star with Einstein-Maxwell equations in general relativity

DOI10.1016/j.amc.2012.01.044zbMath1248.83019OpenAlexW2004595185MaRDI QIDQ440702

J. Herrera, H. S. Yoon

Publication date: 19 August 2012

Published in: Applied Mathematics and Computation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.amc.2012.01.044

zbMATH Keywords

general relativitycanonical coordinatessuper-dense starcharged fluids

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Einstein-Maxwell equations (83C22)

Related Items (6)

Some exact relativistic models of electrically charged self-bound stars ⋮ A family of charge analogue of Durgapal solution ⋮ Well-behaved relativistic charged super-dense star models ⋮ An exact solution of perfect fluid in isotropic coordinates, compatible with relativistic modeling of star ⋮ A new well behaved exact solution in general relativity for perfect fluid ⋮ All static charged dust spheres in general relativity

Cites Work

• Unnamed Item
• Well behaved class of charge analogue of heintzmann's relativistic exact solution
• New class of regular and well behaved exact solutions in general relativity
• Charged analogue of Whittaker's interior solution
• Nonsingular charged analogues of Schwarzschild's interior solution
• Some new static charged spheres
• Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
• A class of charged analogues of Durgapal and Fuloria superdense star
• A superdense star model as charged analogue of Schwarzschild's interior solution
• Tikekar superdense stars in electric fields

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