标题： 非广义Kaniadiakis熵下的范德瓦尔斯黑洞热力学 显示英文标题

标题： Thermodynamics of the Van der Waals black hole within nonextensive Kaniadiakis entropy

摘要： 在本工作中，我们研究了非广延Kaniadakis熵框架下的范德瓦尔斯黑洞的热力学性质。我们表明，黑洞的性质，如质量与温度，与使用玻尔兹曼-吉布斯方法得到的结果不同。此外，非广延性\k{appa}-参数通过引入热力学不稳定性改变了吉布斯自由能的行为，而发射率仅受\k{appa}的影响在低频下。尽管如此，压力-体积（P(V)）特性被发现与\k{appa}和熵形式无关，这与其他反德西特（AdS）黑洞模型不同。总之，所呈现的发现部分支持Gohar和Salzano之前的论点，即在某些情况下所有熵模型是等价且无法区分的[1]。 显示英文摘要

摘要： In this work, we have studied the thermodynamic properties of the Van der Waals black hole in the framework of the nonextensive 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 nonextensivity \k{appa}-parameter changes behavior of the Gibbs free energy via introduced thermodynamic instabilities, whereas the emission rate is influenced by \k{appa} only at low frequencies. Nonetheless, the pressure-volume (P(V)) characteristics are found independent of \k{appa} and the entropy form, unlike in other anti-de Sitter (AdS) black hole models. In summary, presented findings partially support previous arguments of Gohar and Salzano that under certain circumstances all entropic models are equivalent and indistinguishable [1].