Spin-3/2 perturbations of the Kerr-Newman solution

Details Spin-3/2 perturbations of the Kerr-Newman solution Spin-3/2 perturbations of the Kerr-Newman solution

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..46.5395t&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 46, Issue 12, 15 December 1992, pp.5395-5398

Physics

5

Exact Solutions, Supergravity

Scientific paper

The equations for the spin-3/2 perturbations of a rotating charged black hole given by the linearized O(2) extended supergravity model are solved, expressing their complete solution in terms of two Debye potentials that obey the same differential equation. The equation governing the radial parts of the Debye potentials is transformed into a Schrödinger-type equation with a short-range real potential. It is also shown that there exist spin-3/2 perturbations corresponding only to ingoing or only to outgoing waves.

Affiliated with

Also associated with

No associations

Rating

Spin-3/2 perturbations of the Kerr-Newman solution does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spin-3/2 perturbations of the Kerr-Newman solution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spin-3/2 perturbations of the Kerr-Newman solution will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1141330