标题： 蒸发量子温润黑洞的最终状态来自量子标量场的反作用校正 显示英文标题

标题： Evaporating Quantum Lukewarm Black Holes Final State From Back-Reaction Corrections of Quantum Scalar Fields

摘要： 我们获得了无质量、无电荷的动力学量子标量场的重整化应力张量，该场与球对称静态 lukewarm 黑洞最小耦合。 在二维类比中，最小耦合退化为共形耦合，并发现应力张量由异常迹的非局域贡献和一些与 Christensen 和 Fulling 提出的工作密切相关的附加参数决定。 lukewarm 黑洞是一类特殊的 Reissner-Nordström-de Sitter 时空，其中其电荷等于质量。 拥有获得的重整化应力张量后，我们试图得到著名的度规反作用方程的一个时间无关解。 数学推导预测，蒸发量子 lukewarm 黑洞的最终状态会退化为一个具有移动视界位置的稳定微型黑洞。 即扰动的黑洞（宇宙学）视界被压缩（扩展）到小于（大于）相应经典事件视界半径的尺度上。 因此，没有得出对宇宙传感器假说的偏差。 显示英文摘要

摘要： We obtain renormalized stress tensor of a mass-less, charge-less dynamical quantum scalar field, minimally coupled with a spherically symmetric static Lukewarm black hole. In two dimensional analog the minimal coupling reduces to the conformal coupling and the stress tensor is found to be determined by the nonlocal contribution of the anomalous trace and some additional parameters in close relation to the work presented by Christensen and Fulling. Lukewarm black holes are a special class of Reissner- Nordstr\"{o}m-de Sitter space times where its electric charge is equal to its mass. Having the obtained renormalized stress tensor we attempt to obtain a time-independent solution of the well known metric back reaction equation. Mathematical derivations predict that the final state of an evaporating quantum Lukewarm black hole reduces to a remnant stable mini black hole with moved locations of the horizons. Namely the perturbed black hole (cosmological) horizon is compressed (extended) to scales which is smaller (larger) than the corresponding classical radius of the event horizons. Hence there is not obtained an deviation on the cosmic sensor-ship hypothesis.