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- W2783178622 abstract "We compute the mass-to-radius profiles for dark matter admixed strange quark stars in the Starobinsky model of modified gravity. For quark matter, we assume the MIT bag model, while self-interacting dark matter inside the star is modeled as a Bose-Einstein condensate with a polytropic equation of state. We numerically integrate the structure equations in the Einstein frame, adopting the two-fluid formalism, and we treat the curvature correction term nonperturbatively. The effects on the properties of the stars of the amount of dark matter as well as the higher curvature term are investigated. We find that strange quark stars (in agreement with current observational constraints) with the highest masses are equally affected by dark matter and modified gravity." @default.
- W2783178622 created "2018-01-26" @default.
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- W2783178622 date "2018-01-24" @default.
- W2783178622 modified "2023-09-29" @default.
- W2783178622 title "Dark matter admixed strange quark stars in the Starobinsky model" @default.
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- W2783178622 doi "https://doi.org/10.1103/physrevd.97.024030" @default.
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