Non Rindler horizons and radiating black holes

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