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.
Interpretation of the nonex- tensivity parameter q in some applications of Tsallis statistics and Lévy distributions
3 Pith papers cite this work, alongside 673 external citations. Polarity classification is still indexing.
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Hyperstatistics is a renamed gamma-superstatistics result: Laplace-transforming a gamma distribution of inverse temperatures yields the q-exponential, and the paper fits this form to Brownian VACF data without reconciling q and n.
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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.
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A few remarks on hyperstatistics and some applications
Hyperstatistics is a renamed gamma-superstatistics result: Laplace-transforming a gamma distribution of inverse temperatures yields the q-exponential, and the paper fits this form to Brownian VACF data without reconciling q and n.
- Hyperstatistics