The influence of a net charge on the critical mass of a neutron star
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Publication:786600
DOI10.1007/BF00648990zbMath0528.76054MaRDI QIDQ786600
Publication date: 1982
Published in: Astrophysics and Space Science (Search for Journal in Brave)
critical masscharge density assumed proportional to matter densitycompletely degenerate Fermi gasmodified Oppenheimer- Volkoff equationsstructure of spherically symmetric charged star
Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)
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OF CHARGED STARS AND CHARGED BLACK HOLES ⋮ Relativistic charged spheres: compact stars, compactness and stable configurations ⋮ Does charge contribute to the frame dragging of spacetime? ⋮ THE EQUILIBRIUM STRUCTURE OF CHARGED ROTATING RELATIVISTIC STARS ⋮ Role of modified scalar variables in the modeling of spherical fluids ⋮ Shear and expansion evolution for dissipative fluids ⋮ Compact stars described by a charged model ⋮ Detecting vector charge with extreme mass ratio inspirals onto Kerr black holes ⋮ Constraining the electric charges of some astronomical bodies in Reissner-Nordström spacetimes and generic \(r ^{ - 2}\)-type power-law potentials from orbital motions ⋮ Variations in the expansion and shear scalars for dissipative fluids ⋮ Electrically charged strange quark stars with anisotropic matter: exact analytical solution ⋮ Analytic neutron stars in general relativity: Exact solutions for the nonhomogeneous charged model ⋮ Weakly charged compact stars in f(R) gravity
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