标题： 圈量子引力中的准正则模式和视界面面积量子化 显示英文标题

标题： Quasinormal modes and horizon area quantisation in Loop Quantum Gravity

摘要： 有人认为，只要视界是孤立的且Barbero-Immirzi参数为$\gamma \approx \sqrt{3}/6$（与从Bekenstein-Hawking视界熵推导出的值一致），黑洞视界的相邻高次准正规模之间的面积量子就与环圈量子引力预测的面积间隙相一致。 显示英文摘要

摘要： It is argued that the quantum of area between consecutive, high overtones quasinormal modes of a black hole horizon coincides with the area gap predicted by Loop Quantum Gravity, as long as the horizon is isolated and the Barbero-Immirzi parameter is $\gamma \approx \sqrt{3}/6$, in agreement with the value derived from the Bekenstein-Hawking horizon entropy.