Compact stars described by a charged model

DOI10.1142/S0218271820500224zbMath1434.85008OpenAlexW2999447424WikidataQ126402198 ScholiaQ126402198MaRDI QIDQ5109439

Arthur Cleary-Balderas, Rafael Soto-Espitia, Joaquin Estevez-Delgado, Aurelio Taméz Murguía

Publication date: 12 May 2020

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271820500224

zbMATH Keywords

compact starscharged perfect fluidspherically symmetric exact solutions

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Einstein-Maxwell equations (83C22)

Related Items (5)

An anisotropic charged fluids with Chaplygin equation of state ⋮ Relativistic charged stellar modeling with a perfect fluid sphere ⋮ A quintessence type interior solution with Karmarkar condition ⋮ An anisotropic model for represent compact stars ⋮ An isotropic analytical model for charged stars

Cites Work

• Well behaved class of charge analogue of heintzmann's relativistic exact solution
• Charge analogue of Tolman IV solution for anisotropic fluid
• The influence of a net charge on the critical mass of a neutron star
• Equilibrium of a static charged perfect fluid sphere
• 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
• Relativistic modelling of a superdense star containing a charged perfect fluid
• A family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativity
• General Relativistic Fluid Spheres
• Sharp bounds on the radius of relativistic charged spheres: Guilfoyle's stars saturate the Buchdahl–Andréasson bound
• A singularity-free solution for a charged fluid sphere in general relativity
• Compact stars
• Analysis of charged compact stars in modified gravity
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• A regular perfect fluid model for dense stars
• General Relativity

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