ON HAWKING RADIATION AS TUNNELING WITH BACK-REACTION

By A. Medved, E. Vagenas. 2005

203 citations recorded by the source corpus.

Recently, Angheben et al.1 have presented a refined method for calculating the (tree-level) black hole temperature by way of the tunneling paradigm. Here, we demonstrate how their formalism can be suitably adapted to accommodate the (higher-order) effects of the gravitational back-reaction.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/bedd62a31e2263f29ca2941fe3d8bc783ade5227

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Citations in the corpus

Fermions tunnelling from black holes (2007, methodology): “In various scalar field cases this is inherent in the Parikh/Wilczek tunnelling method [3, 7–18] and can be incorporated into the Hamilton–Jacobi tunnelling approach [6].”
Charged fermions tunnelling from Kerr–Newman black holes (2008, unknown): “A 0 B 0 exp [ i ~ I ] we find upon insertion into the (chargeless) Dirac equation (5) we obtain −B ( 1√ f ∂tI + √ g∂rI ) +Am = 0 (33) −B ( i √ f FK ∂φI − i H√ FK ∂tI + 1√ Σ ∂θI ) = 0 (34) A ( 1√ f ∂tI − √ g∂rI ) +Bm = 0 (35) −A ( i √ f FK ∂φI − i H√ FK ∂tI + 1√ Σ ∂θI ) = 0 (36) Repeating the…”