In this article the characterization of the separation constant for the spin one and gravitational perturbations in Kerr geometry are given. The characterization is given for the corresponding Hertz potentials and induced for the corresponding vector and metric perturbations using the results of Cohen and Kegeles.
|Original language||English (US)|
|Number of pages||10|
|Journal||Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences|
|State||Published - 1996|