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- W3092235877 endingPage "2050216" @default.
- W3092235877 startingPage "2050216" @default.
- W3092235877 abstract "This paper is devoted to formulate a new model of quintessence anisotropic compact stars in the modified [Formula: see text] gravity. Dynamical equations in modified theory consisting of anisotropic fluid along with quintessence field have been evaluated by adopting analytical solution of Krori–Barua. In order to determine the unknown constraints of Krori–Barua metric observational data of different stars, [Formula: see text]-[Formula: see text], [Formula: see text], [Formula: see text]-[Formula: see text] has been taken into account. To solve the dynamical equations Starobinsky-like model, [Formula: see text] of modified gravity has been used. The outcome of the results depicts that all the examined celestial bodies are free from central singularity and are physically stable. Different physical parameters, such as energy density, energy conditions, evolution of quintessence and compactness factor, have been reviewed in detail." @default.
- W3092235877 created "2020-10-15" @default.
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- W3092235877 date "2020-11-18" @default.
- W3092235877 modified "2023-09-30" @default.
- W3092235877 title "Anisotropic strange quintessence stars in f(R,G) gravity" @default.
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- W3092235877 doi "https://doi.org/10.1142/s0219887820502163" @default.
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