论文标题
tsallis统计力学中的鹰辐射的光谱
The spectrum of Hawking radiation in Tsallis statistical mechanics
论文作者
论文摘要
霍金辐射是现代感激理论中的核心之一。几篇文章计算了Boltzmann-Gibbs统计力学中鹰辐射的范围。但是，根据最近的研究，标准统计力学无法研究重力系统。在本文中，我们计算了Tsallis统计力学中鹰辐射范围的修改。我们获得了修改后的Stefan-Boltzmann定律和霍金辐射的修改能力。我们证实了GIDDING提出的结论，即辐射应源于有效半径，该半径延伸到黑洞的地平线之外。还讨论了黑洞的寿命和大Q的效果。
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.
