Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
1998-01-13
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
12 pages, latex
Scientific paper
We show that a surface term should be added to the Einstein-Hilbert action in order to properly describe quantum transitions occurring around a black hole. The introduction of this boundary term has been advocated by Teitelboim and collaborators and it has been used in the computation of the black hole entropy. Here, we use it to compute the gravitational corrections to the transition amplitudes giving rise to Hawking radiation. This surface term implies that the probability to emit a particle is given by $e^{- \Delta A/4}$ where $\Delta A$ is the change in the area of the black hole horizon induced by the emission. Its inclusion at the level of the amplitudes therefore relates quantum black hole radiation to the first law of black hole dynamics. In both cases indeed, the term expressing the change in area directly results from the same boundary term introduced for the same reason: to obtain a well defined action principle.
Massar Serge
Parentani Renaud
No associations
LandOfFree
On the Gravitational Back Reaction to Hawking Radiation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the Gravitational Back Reaction to Hawking Radiation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Gravitational Back Reaction to Hawking Radiation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-644207