TL;DR
This paper discusses a method for remotely sensing the temperature distribution of small black holes by analyzing their Hawking grey pulses using a modified Moebius inverse transform.
Contribution
It introduces the application of Chen's modified Moebius inverse transform to black hole spectral data for surface temperature estimation.
Findings
Demonstrates the feasibility of spectral analysis for black hole temperature mapping
Provides a mathematical framework for interpreting Hawking grey pulses
Suggests potential for remote black hole diagnostics
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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