In this work we construct metrics corresponding to radiating black holes whose near horizon regions cannot be approximated by Rindler space–time. We first construct infinite parameter coordinate transformations from Minkowski coordinates, such that an observer using these coordinates to describe space–time events measures the Minkowski vacuum to be Planckian. Utilizing these results, we construct a family of black holes that radiate at spatial infinity. As an illustration, we study a subset of the black hole solutions and show that they satisfy the null energy condition.

中文翻译：

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非林德勒视界和辐射黑洞

在这项工作中，我们构建了对应于辐射黑洞的度量，这些黑洞的近视界区域不能用 Rindler 时空近似。我们首先从 Minkowski 坐标构造无限参数坐标变换，以便使用这些坐标来描述时空事件的观察者将 Minkowski 真空测量为普朗克。利用这些结果，我们构建了一个以无限空间辐射的黑洞家族。作为说明，我们研究了黑洞解的一个子集，并表明它们满足零能量条件。