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Quantum Fields in Curved Space

N. D. Birrell, +1 more
- pp 349
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TLDR
A comprehensive review of the subject of gravitational effects in quantum field theory can be found in this paper, where special emphasis is given to the Hawking black hole evaporation effect, and to particle creation processes in the early universe.
Abstract
This book presents a comprehensive review of the subject of gravitational effects in quantum field theory. Although the treatment is general, special emphasis is given to the Hawking black hole evaporation effect, and to particle creation processes in the early universe. The last decade has witnessed a phenomenal growth in this subject. This is the first attempt to collect and unify the vast literature that has contributed to this development. All the major technical results are presented, and the theory is developed carefully from first principles. Here is everything that students or researchers will need to embark upon calculations involving quantum effects of gravity at the so-called one-loop approximation level.

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Initial state of matter fields and trans-Planckian physics: Can CMB observations disentangle the two?

TL;DR: In this article, it was shown that the standard, scale-invariant, inflationary perturbation spectrum can be modified if the effects of trans-planckian physics are incorporated into the dynamics of the matter field in a phenomenological manner, by the modification of the dispersion relation.
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Notes on Semiclassical Gravity

TL;DR: In this article, the authors investigated the different possible ways of defining the semiclassical limit of quantum general relativity and developed rules for finding the back-reaction of the quantum mode q on the classical mode Q, which can be found using the phase of the wave function which describes the dynamics of q.
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Entropy of a quantum field in rotating black holes.

Min-Ho Lee, +1 more
- 15 Sep 1996 - 
TL;DR: By using the brick wall method, a free energy and the entropy of the scalar field in rotating black holes are calculated as one approaches the stationary limit surface rather than the event horizon in a comoving frame.
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Physical observability of horizons

TL;DR: In this paper, it was shown that the only situation in which an event horizon becomes physically observable is for the very highly idealized stationary or static black holes, when the event horizon is a Killing horizon which is degenerate with the apparent and trapping horizons, and then it is the physical observability of the apparent/trapping horizons that is fundamental.
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Backreaction of Hawking Radiation on a Gravitationally Collapsing Star I: Black Holes?

TL;DR: In this paper, the authors investigated the back-reaction of Hawking radiation on the interior of a gravitationally collapsing star, in a Hartle-Hawking initial vacuum, and showed that due to the negative energy Hawking radiation in the interior, the collapse of the star stops at a finite radius, before the singularity and the event horizon of a black hole have a chance to form.
References
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Particle Creation by Black Holes

TL;DR: In this article, it is shown that quantum mechanical effects cause black holes to create and emit particles as if they were hot bodies with temperature, which leads to a slow decrease in the mass of the black hole and to its eventual disappearance.
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Propagateurs et commutateurs en relativité générale

TL;DR: In this paper, the authors present conditions générales d'utilisation (http://www.numdam.org/conditions), i.e., Toute copie ou impression de ce fichier doit contenir la présente mention de copyright.
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Foundations of the Theory of Dynamical Systems of Infinitely Many Degrees of Freedom, II

TL;DR: The notion of quantum field remains at this time still rather elusive from a rigorous standpoint as mentioned in this paper, and it was recognized very early by Bohr and Rosenfeld that even in the case of a free field, no physical meaning could be attached to the values of the field at a particular point, only the suitably smoothed averages over finite space-time regions had such a meaning.
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Evidence for the existence of gravitational radiation from measurements of the binary pulsar psr 1913+16

TL;DR: The results of four years of timing observations of PSR 1913+16 made with the 305m telescope at the Arecibo Observatory at frequencies near 430 and 1410 MHz are summarized in this paper.
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