The bounded discrete thermal weight suppresses black-hole Hawking luminosity near the cutoff and supports an exact Jarzynski identity for work but not a simple Crooks relation.
The numerical coefficient is not universal (it depends on the constant-absorption s-wave approxima- tion), but the negative sign and the linear scaling with bkBTH are robust
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Bounded thermal weights from a discrete Boltzmann factor
The bounded discrete thermal weight suppresses black-hole Hawking luminosity near the cutoff and supports an exact Jarzynski identity for work but not a simple Crooks relation.