论文标题
回路量子重力中的准模式和地平线面积定量
Quasinormal modes and horizon area quantisation in Loop Quantum Gravity
论文作者
论文摘要
有人认为，只要隔离地平线并且Barbero-immirzi参数为$γ\ op sqrt {3} {3}/6 $，与该数值脱离了数值，那么黑洞地平线的连续连续高覆层的准覆质模式之间的量子与由环量子重力预测的面积间隙相吻合就与面积差距相吻合。
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 $γ\approx \sqrt{3}/6$, in agreement with the value derived from the Bekenstein-Hawking horizon entropy.
