Entropy of a radiating rotating charged black hole

Details Entropy of a radiating rotating charged black hole Entropy of a radiating rotating charged black hole

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21.2595w&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 11, pp. 2595-2602 (2004).

Physics

4

Scientific paper

The Hawking radiation temperature and the entropy of a radiating rotating charged black hole are calculated by employing the method of tortoise coordinate transformation and the improved brick-wall model. A new tortoise coordinate transformation is introduced which simplifies the cut-off factor and more satisfying results are obtained. The results show that the temperature of the event horizon depends on time and angle, and the entropy of a non-stationary black hole is exactly proportional to its horizon area as in the case of a stationary black hole.

Affiliated with

Also associated with

No associations

Rating

Entropy of a radiating rotating charged 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 Entropy of a radiating rotating charged black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Entropy of a radiating rotating charged black hole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-891671