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• W2897580929 abstract "We present interesting aspects of neutron stars (NSs) from the standpoint of a modified theory of gravity called Hoifmmode check{r}else v{r}fi{}ava-Lifshitz (HL) gravity. A deviation from general relativity (GR) in HL gravity can change typical features of the NS structure. In this study, we investigate the NS structure by deriving the Tolman-Oppenheimer-Volkoff equation in HL gravity. We find that a NS in HL gravity with a larger radius and heavier mass than a NS in GR remains stable without collapsing into a black hole." @default.
• W2897580929 created "2018-10-26" @default.
• W2897580929 creator A5007052631 @default.
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• W2897580929 creator A5070829020 @default.
• W2897580929 date "2021-02-24" @default.
• W2897580929 modified "2023-10-15" @default.
• W2897580929 title "Neutron star structure in Hořava-Lifshitz gravity" @default.
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• W2897580929 doi "https://doi.org/10.1103/physrevd.103.044052" @default.
• W2897580929 hasPublicationYear "2021" @default.
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