A look into the mass–radius relation of the neutron star in modified Chaplygin gas background

DOI10.1142/S0219887822500657OpenAlexW4210747748MaRDI QIDQ6196420

Surajit Chattopadhyay, Unnamed Author, Unnamed Author

Publication date: 14 March 2024

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

Full work available at URL: https://doi.org/10.1142/s0219887822500657

zbMATH Keywords

neutron star\(f(R)\) gravitymodified Chaplygin gasTolman-Oppenheimer-Volkoff equation

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Unnamed Item
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• Modified Chaplygin gas cosmology
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• The realistic models of relativistic stars in f  ( R ) = R + αR ² gravity
• Role of modified Chaplygin gas in accelerated universe
• Cyclotron harmonics in opacities of isolated neutron star atmospheres
• Modified Chaplygin gas equation of state on viscous dissipative extended holographic Ricci dark energy and the cosmological consequences
• On Massive Neutron Cores
• An alternative to quintessence

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