Thermodynamic properties of the blackbody radiation: A Kaniadakis approach

被引:16
|
作者
Lourek, Imene [1 ]
Tribeche, Mouloud [1 ,2 ]
机构
[1] Univ Bab Ezzouar, USTHB, PPG, Fac Phys,TPL, BP 32, Algiers 16111, Algeria
[2] Algerian Acad Sci & Technol, Algiers, Algeria
关键词
Thermodynamic properties; Blackbody radiation; kappa-Statistics; Kaniadakis; STELLAR ROTATIONAL VELOCITIES; PERSONAL INCOME-DISTRIBUTION; KAPPA-DEFORMED STATISTICS; RANDOM-MATRIX THEORY; GENERALIZED DISTRIBUTION; TSALLIS STATISTICS; BODY RADIATION; LAW; ENTROPY; FIELD;
D O I
10.1016/j.physleta.2016.12.019
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The thermodynamic properties of the blackbody radiation are revisited, for the first time, within the theoretical framework of the kappa-statistics introduced by Kaniadakis. Using the epsilon-counterpart of the Bose-Einstein distribution, generalized expressions for the free energy, the entropy, the specific heat, and the pressure are obtained. All quantities are shown to recover their standard expressions in the limit kappa -> 0. The reexamination of the thermodynamic properties of the blackbody radiation shows that it emits more energy with an increase of the value of vertical bar kappa vertical bar in comparison with the standard Planck radiation law. Moreover, the effects of the deformed Kaniadakis statistics are shown to be more appreciable for high temperatures. Our results could be used as a theoretical support for experimental studies implying blackbody radiation such as the study of microwave background radiation. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:452 / 456
页数:5
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