Kaczmarek Adam Z, Sekhmani Yassine, Szczȩśniak Dominik, Rayimbaev Javlon
Institute of Physics, Faculty of Science and Technology, Jan Długosz University in Czestochowa, 13/15 Armii Krajowej Ave., 42200 Czestochowa, Poland.
Center for Theoretical Physics, Khazar University, 41 Mehseti Street, Baku AZ1096, Azerbaijan.
Entropy (Basel). 2024 Nov 27;26(12):1027. doi: 10.3390/e26121027.
In this work, we have studied the thermodynamic properties of the Van der Waals black hole in the framework of the relativistic Kaniadakis entropy. We have shown that the black hole properties, such as the mass and temperature, differ from those obtained by using the the Boltzmann-Gibbs approach. Moreover, the deformation κ-parameter changes the behavior of the Gibbs free energy via introduced thermodynamic instabilities, whereas the emission rate is influenced by κ only at low frequencies. Nonetheless, the pressure-volume (P(V)) characteristics are found independent of κ and the entropy form, unlike in other anti-de Sitter (AdS) black hole models. In summary, the presented findings partially support the previous arguments of Gohar and Salzano that, under certain circumstances, all entropic models are equivalent and indistinguishable.
在这项工作中，我们在相对论性卡尼亚达基斯熵的框架下研究了范德瓦尔斯黑洞的热力学性质。我们已经表明，黑洞的性质，如质量和温度，与使用玻尔兹曼-吉布斯方法得到的性质不同。此外，变形κ参数通过引入的热力学不稳定性改变了吉布斯自由能的行为，而发射率仅在低频时受κ影响。尽管如此，与其他反德西特（AdS）黑洞模型不同，压力-体积（P(V)）特性被发现与κ和熵的形式无关。总之，本文的研究结果部分支持了戈哈尔和萨尔扎诺之前的观点，即在某些情况下，所有熵模型都是等效且不可区分的。
