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On the remote sensing of Hawking grey pulses

H. C. Rosu

gr-qcarXiv:gr-qc/9408039

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

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