Phys. Rev. D 67, 064021 (2003) [6 pages]Explicit solutions to the time-independent perturbation equations of the Reissner-Nordström geometryReceived 31 October 2002; published 28 March 2003 It is proven that the equations for the time-independent, negative-parity, gravitational and electromagnetic perturbations of the Reissner-Nordström geometry have (for each angular momentum) one solution in the form of a finite power series in the (Schwarzschild-like) radial coordinate r. The explicit form of these solutions is given. Therefrom the second fundamental solutions of these equations, and the positive-parity perturbations, can also be constructed explicitly. © 2003 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.67.064021
DOI:
10.1103/PhysRevD.67.064021
PACS:
04.25.Nx, 04.70.-s
|
|
About | Terms and Conditions | Subscriptions | Search | Help
Use of the American Physical Society websites and journals implies that the user has read and agrees to our Terms and Conditions and any applicable Subscription Agreement. Physical Review®, Physical Review Letters®, Reviews of Modern Physics®, and Physical Review Special Topics® are trademarks of the American Physical Society.