Quasi-normal modes of the Kerr-Newman black hole.

Details Quasi-normal modes of the Kerr-Newman black hole. Quasi-normal modes of the Kerr-Newman black hole.

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ncimb.108..991k&link_type=abstract

Nuovo Cimento B, Vol. 108, No. 9, p. 991 - 998

Physics

17

Black Holes: Frequency

Scientific paper

The quasi-normal frequencies of the Kerr-Newman black hole are calculated using a well-known WKB semi-analytic method. It is the first time that quasi-normal frequencies for the Kerr-Newman black hole are ever calculated by any method. The author considers perturbations with a frozen Maxwell field and a perturbed Einstein field. He was led to such a consideration, because, for combined perturbations of both fields, the equations do not decouple.

Affiliated with

Also associated with

No associations

Rating

Quasi-normal modes of the Kerr-Newman black hole. 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 Quasi-normal modes of the Kerr-Newman black hole., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quasi-normal modes of the Kerr-Newman black hole. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1565371