dc.creatorMartínez, S.
dc.creatorPennini, Flavia
dc.creatorTessone, Claudio J.
dc.creatorPlastino, Ángel Luis
dc.date2002
dc.date2022-03-10T16:28:40Z
dc.date.accessioned2023-07-15T04:18:31Z
dc.date.available2023-07-15T04:18:31Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/132352
dc.identifierissn:0378-4371
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7469048
dc.descriptionWe give an exact information-theory treatment of the n-dimensional black-body radiation process in a non-extensive scenario. We develop a q-generalization of the laws of (i) Stefan–Boltzmann, (ii) Planck, and (iii) Wien, and show that conventional, canonical results are obtained at temperatures above 1 K. Classical relationships between radiation, pressure, and internal energy are recovered (independently of the q value). Analyzing the particles’ density for q ≈ 1, we see that the non-extensive parameter q introduces a 9ctitious chemical potential. We apply our results to experimental data on the cosmic microwave background and reproduce it with acceptable accuracy for di:erent temperatures (each one associated to a particular q value).
dc.descriptionInstituto de Física La Plata
dc.formatapplication/pdf
dc.format85-105
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectFísica
dc.subjectq-Thermostatistics
dc.subjectBlack-body radiation
dc.titleq-Thermostatistics and the black-body radiation problem
dc.typeArticulo
dc.typeArticulo


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