论文标题
碰撞黑洞上的量子头发
Quantum Hair on Colliding Black Holes
论文作者
论文摘要
抽象的黑洞碰撞会产生重力辐射，通常以量子极限为重力。黑洞的拉伸视野包含量子信息或量子头发的形式，在黑洞的合并中，它们参与了重力。这可以通过类似于BOHR的黑洞（BH）量子物理学的方法来促进，以BH量子力学的方法（QNM）方法。量子重力和事件范围内的量子头发对BH结合中的较高能量感到兴奋。在碰撞之前，两个BHS的近地平线条件是一个变形的广告时空。这些激发的BH量子头发的激发态随着重力的产生而放松。然后说这是为了定义地平线上的量子头发给出的RT熵。然后，来自BH结合的这些信息量位应在重力波（GW）数据中出现。这是标准ADS/CFT对应关系和Ryu-Takayanagi（RT）公式的一种形式。
Abstract Black hole collision produce gravitational radiation which is generally thought in a quantum limit to be gravitons. The stretched horizon of a black hole contains quantum information, or a form of quantum hair, which in a coalescence of black holes participates in the generation of gravitons. This may be facilitated with a Bohr-like approach to black hole (BH) quantum physics with quasi-normal mode (QNM) approach to BH quantum mechanics. Quantum gravity and quantum hair on event horizons is excited to higher energy in BH coalescence. The near horizon condition for two BHs right before collision is a deformed AdS spacetime. These excited states of BH quantum hair then relax with the production of gravitons. This is then argued to define RT entropy given by quantum hair on the horizons. These qubits of information from a BH coalescence should then appear in gravitational wave (GW) data. This is a form of the standard AdS/CFT correspondence and the Ryu-Takayanagi (RT) formula.
