Thermality of the Hawking flux
Matt Visser (Victoria University of Wellington)

TL;DR
This paper critically examines whether the Hawking radiation from black holes is truly thermal, emphasizing the importance of correlations and the limitations of the classical thermodynamic analogy in quantum contexts.
Contribution
It clarifies the assumptions behind the thermality of Hawking flux, highlighting that it is only approximately Planckian and may include correlations, challenging common simplifications.
Findings
Hawking flux is only approximately Planck-shaped within a bounded frequency range.
Standard physics bounds the frequency range of the Hawking radiation.
There is no fundamental reason to assume Hawking photons are uncorrelated.
Abstract
Is the Hawking flux "thermal"? Unfortunately, the answer to this seemingly innocent question depends on a number of often unstated, but quite crucial, technical assumptions built into modern (mis-)interpretations of the word "thermal". The original 1850's notions of thermality --- based on classical thermodynamic reasoning applied to idealized "black bodies" or "lamp black surfaces" --- when supplemented by specific basic quantum ideas from the early 1900's, immediately led to the notion of the black-body spectrum, (the Planck-shaped spectrum), but "without" any specific assumptions or conclusions regarding correlations between the quanta. Many (not all) modern authors (often implicitly and unintentionally) add an extra, and quite unnecessary, assumption that there are no correlations in the black-body radiation; but such usage is profoundly ahistorical and dangerously misleading.…
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