标题： 霍金辐射在塔尔塞利统计力学中的谱 显示英文标题

标题： The spectrum of Hawking radiation in Tsallis statistical mechanics

摘要： 霍金辐射是现代引力理论的核心之一。 几篇文章已经计算了霍金辐射在玻尔兹曼-吉布斯统计力学中的谱。 然而，根据最近的研究，引力系统不能通过标准统计力学来研究。 在本文中，我们计算了霍金辐射谱在塔拉西统计力学中的修正。 我们得到了修正后的斯特藩-玻尔兹曼定律和修正后的霍金辐射功率。 我们确认了吉丁斯提出的结论，即辐射应起源于有效半径，该半径远远超出黑洞视界的范围。 还讨论了黑洞的寿命和大q的影响。 显示英文摘要

摘要： Hawking radiation is one of the cores in modern gratitational theory. Several articles have calculated the spectrum of Hawking radiation in Boltzmann-Gibbs statistical mechanics. However, based on recent researches, gravitational systems cannot be studied by the standard statistical mechanics. In this article, we calculate the modification to the spectrum of Hawking radiation in Tsallis statistical mechanics. We obtain the modified Stefan-Boltzmann's law and modified power of Hawking radiation. We confirm the conclusion proposed by Giddings, namely, the radiation should originate from the effective radius, which extends well outside the horizon of black-hole. The lifetime of black hole and the effect of large q are discussed as well.