Moebius Inverse Problem for Distorted Black Holes

Details Moebius Inverse Problem for Distorted Black Holes Moebius Inverse Problem for Distorted Black Holes

1995-11-03

arxiv.org/abs/gr-qc/9511013v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

2+10 Latex pages, corrected and updated version of Nuovo Cimento B 108, 1333 (1993), no figures, accompanying file is gr-qc/94

Scientific paper

Hawking ``thermal'' radiation could be a means to detect black holes of micron sizes, which may be hovering through the universe. We consider these micro-black holes to be distorted by the presence of some distribution of matter representing a convolution factor for their Hawking radiation. One may hope to determine from their Hawking signals the temperature distribution of their material shells by the inverse black body problem. In 1990, Nan-xian Chen has used a so-called modified M\"{o}bius transform to solve the inverse black body problem. We discuss and apply this technique to Hawking radiation of distorted micro-black holes. Some comments on supersymmetric applications of M\"{o}bius function and transform are also added.

Affiliated with

Also associated with

No associations

Rating

Moebius Inverse Problem for Distorted Black Holes 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 Moebius Inverse Problem for Distorted Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Moebius Inverse Problem for Distorted Black Holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-87968