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.
Hawking Radiation of Weyl Neutrinos in a Rectilinearly Non-uniformly Accelerating Kinnersley Black Hole
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abstract
Quantum thermal effect of Weyl neutrinos in a rectilinearly non-uniformly accelerating Kinnersley black hole is investigated by using the generalized tortoise coordinate transformation. The equation that determines the location, the Hawking temperature of the event horizon and the thermal radiation spectrum of neutrinos are derived. Our results show that the location and the temperature of the event horizon depend not only on the time but also on the angle.
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gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
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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.