SEMICLASSICAL METHODS FOR HAWKING RADIATION FROM A VAIDYA BLACK HOLE

DOI10.1142/S0217751X1004749XzbMath1184.83033arXiv0908.2895MaRDI QIDQ3553610

Haryanto M. Siahaan, Triyanta

Publication date: 21 April 2010

Published in: International Journal of Modern Physics A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0908.2895

zbMATH Keywords

Hawking radiationsemiclassical methodVaidya black holestunneling pictures

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20)

Related Items (6)

Accelerating black holes in the low energy heterotic string theory ⋮ On the photon motion near a five-dimensional Schwarzschild black hole ⋮ Evaporation of Dynamical Horizon with the Hawking Temperature in the K‐essence Emergent Vaidya Spacetime ⋮ A model of the collapse and evaporation of charged black holes ⋮ Hidden conformal symmetry for the accelerating Kerr black holes ⋮ Quantum tunnelling for Hawking radiation from both static and dynamic black holes

Cites Work

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• THERMAL RADIATION OF VARIOUS GRAVITATIONAL BACKGROUNDS
• Hawking radiation in different coordinate settings: complex paths approach
• Hawking Radiation As Tunneling
• Production and decay of evolving horizons
• ON HAWKING RADIATION AS TUNNELING WITH BACK-REACTION
• General Relativity

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