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- W4382319345 abstract "In this paper, we study the slowly rotating neutron stars in $f(R, T)$ gravity based on Hartle-Thorne formalism. We compute the mass, radius, moment of inertia, change in radius and binding energy due to rotation, eccentricity, quadrupole moment and the tidal love number. The quantities, which are of the second order in angular velocity, like, change in radius and binding energy due to rotation, eccentricity and quadrupole moment, deviate more from their corresponding general relativistic counterparts in lighter neutron stars than heavier ones. Whereas the moment of inertia, which is of the first order in angular velocity, in $f(R, T)$ gravity, slightly diverges from the general relativistic one. The Equation of state-independent I-Love-Q relation retains in $f(R, T) $ gravity, and it coincides with the general relativistic ones within less than one percent even for the maximum allowed coupling parameters." @default.
- W4382319345 created "2023-06-28" @default.
- W4382319345 creator A5052427954 @default.
- W4382319345 creator A5067080947 @default.
- W4382319345 date "2023-06-23" @default.
- W4382319345 modified "2023-10-09" @default.
- W4382319345 title "Neutron Stars In $f(R,T)$ Theory: Slow Rotation Approximation" @default.
- W4382319345 doi "https://doi.org/10.48550/arxiv.2306.13758" @default.
- W4382319345 hasPublicationYear "2023" @default.
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