Perturbations and Gravitomagnetism in the Kerr-Taub-NUT Spacetime

Details Perturbations and Gravitomagnetism in the Kerr-Taub-NUT Spacetime Perturbations and Gravitomagnetism in the Kerr-Taub-NUT Spacetime

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1543b&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

The master equation describing massless fields of different spin in the Kerr-Taub-NUT spacetime representing a source with a mass plus gravitomagnetic monopole and dipole moments is studied. This equation can be separated into its radial and angular parts. The behaviour of the radial functions at infinity and near the horizon can be used to examine the influence of the NUT parameter on the phenomenon of superradiance. Moreover, we discuss the coupling between the spin of the perturbing field and the gravitomagnetic monopole moment.

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