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• W4385741755 endingPage "116325" @default.
• W4385741755 startingPage "116325" @default.
• W4385741755 abstract "The slow rotation of Kerr-NUT spacetime is explored by taking into account the linear form of rotation and NUT parameters in the dynamical Chern-Simon gravity theory, which can be formulated from a scalar field describing the background. We show that in the absence of the potential scalar field, the metric potential does not respect the effect of the NUT parameter, although the scalar field is affected by the rotation and NUT parameters. As a result, unlike the slowly rotating black hole solution presented in [1], the cross term of the metric potential, which has both rotation and NUT parameters, has no contribution up to the leading order of the first order perturbation." @default.
• W4385741755 created "2023-08-11" @default.
• W4385741755 creator A5058447608 @default.
• W4385741755 creator A5081529818 @default.
• W4385741755 date "2023-09-01" @default.
• W4385741755 modified "2023-09-27" @default.
• W4385741755 title "Slow Kerr-NUT black hole solution in dynamical Chern-Simons modified gravity" @default.
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• W4385741755 doi "https://doi.org/10.1016/j.nuclphysb.2023.116325" @default.
• W4385741755 hasPublicationYear "2023" @default.
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