Chaplygin strange stars in presence of quintessence

DOI10.1142/S0217732321502138zbMath1489.85009OpenAlexW3203475478MaRDI QIDQ5067311

Noel Enrique Rodríguez Maya, Arthur Cleary-Balderas, José Martínez Peña, Modesto Pineda Duran, Joaquin Estevez-Delgado

Publication date: 1 April 2022

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

Full work available at URL: https://doi.org/10.1142/s0217732321502138

zbMATH Keywords

exact solutionsChaplygin gasquintessencecompact stars

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Anisotropy in solid mechanics (74E10) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Stability and instability of geophysical and astrophysical flows (76E20) Compactifications; symmetric and spherical varieties (14M27)

Related Items (2)

Determination of the charge for strange stars ⋮ A quintessence type interior solution with Karmarkar condition

Cites Work

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• Some simple predictions from \(E_{11}\) symmetry
• Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
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• Role of modified Chaplygin gas in accelerated universe
• Quintessence and black holes
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• A regular perfect fluid model for dense stars
• General Relativity
• An alternative to quintessence

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