A regular perfect fluid model for dense stars

DOI10.1142/S0217732319501153zbMath1414.85004OpenAlexW2937070166WikidataQ64296734 ScholiaQ64296734MaRDI QIDQ5379253

Modesto Pineda Duran, Joaquin Estevez-Delgado, Jorge Mauricio Paulin-Fuentes, Gabino Estevez-Delgado, Nadiezhda Montelongo García

Publication date: 28 May 2019

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732319501153

zbMATH Keywords

exact solutionsgeneral relativityisotropic perfect fluidrelativistic compact stars

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (13)

An anisotropic charged fluids with Chaplygin equation of state ⋮ Chaplygin strange stars in presence of quintessence ⋮ Determination of the charge for strange stars ⋮ Energy–momentum density and pressure relations for a relativistic ideal gas with a bulk motion ⋮ Relativistic charged stellar modeling with a perfect fluid sphere ⋮ Compact stars described by a charged model ⋮ Description of the interior of the neutron star in EXO 1785-248 by mean of the Karmarkar condition ⋮ A quintessence type interior solution with Karmarkar condition ⋮ A charged perfect fluid solution ⋮ An anisotropic model for represent compact stars ⋮ An anisotropic model for stars ⋮ An interior solution with perfect fluid ⋮ An isotropic analytical model for charged stars

Cites Work

• Unnamed Item
• Well behaved class of charge analogue of heintzmann's relativistic exact solution
• A class of regular and well behaved charge analogue of Kuchowicz's relativistic super-dense star model
• Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
• Relativistic model for anisotropic strange stars
• A family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativity
• Exact solutions to Einstein's field equations for perfect spherically symmetric static fluids
• Compact stars
• Neutron stars structure in the context of massive gravity
• Strange stars inf(R,𝒯) gravity
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• MAXIMUM MASS OF A CLASS OF COLD COMPACT STARS
• Static Solutions of Einstein's Field Equations for Spheres of Fluid

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