On the remote sensing of Hawking grey pulses
arXiv:gr-qc/9408039 · doi:10.1142/S0217732398000759
Abstract
This is a short note on the black hole remote-sensing problem, i.e., finding out `surface' temperature distributions of various types of small (micron-sized) black holes from the spectral measurements of their Hawking grey pulses. Chen's modified Moebius inverse transform is illustrated in this context
4 pages, LaTex, published version