The RVB-residue method is generalized to dynamical black holes, reproducing the local trapping-horizon temperature for Vaidya and yielding a point-dependent temperature for Kinnersley.
Topological approach to derive the global Hawking temperature of massive BTZ black holes,
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Hawking Temperatures of Dynamical Black Holes from the RVB--Residue Method:Vaidya and Kinnersley Geometries
The RVB-residue method is generalized to dynamical black holes, reproducing the local trapping-horizon temperature for Vaidya and yielding a point-dependent temperature for Kinnersley.