On the semiclassical treatment of Hawking radiation
P. Menotti. (2009)cite arxiv:0911.4358
Comment: 18 pages, LaTeX.
Abstract
In the context of the semiclassical treatment of Hawking radiation we prove
the universality of the reduced canonical momentum for the system of a massive
shell self gravitating in a spherical gravitational field within the Painlevé
family of gauges. We show that one can construct modes which are regular on the
horizon both by considering as hamiltonian the exterior boundary term and by
using as hamiltonian the interior boundary term. The late time expansion is
given in both approaches and their time Fourier expansion computed to reproduce
the self reaction correction to the Hawking spectrum.
Description
On the semiclassical treatment of Hawking radiation
%0 Journal Article
%1 Menotti2009
%A Menotti, Pietro
%D 2009
%K black hawking holes radiation
%T On the semiclassical treatment of Hawking radiation
%U http://arxiv.org/abs/0911.4358
%X In the context of the semiclassical treatment of Hawking radiation we prove
the universality of the reduced canonical momentum for the system of a massive
shell self gravitating in a spherical gravitational field within the Painlevé
family of gauges. We show that one can construct modes which are regular on the
horizon both by considering as hamiltonian the exterior boundary term and by
using as hamiltonian the interior boundary term. The late time expansion is
given in both approaches and their time Fourier expansion computed to reproduce
the self reaction correction to the Hawking spectrum.
@article{Menotti2009,
abstract = { In the context of the semiclassical treatment of Hawking radiation we prove
the universality of the reduced canonical momentum for the system of a massive
shell self gravitating in a spherical gravitational field within the Painlev\'e
family of gauges. We show that one can construct modes which are regular on the
horizon both by considering as hamiltonian the exterior boundary term and by
using as hamiltonian the interior boundary term. The late time expansion is
given in both approaches and their time Fourier expansion computed to reproduce
the self reaction correction to the Hawking spectrum.
},
added-at = {2009-11-27T10:52:35.000+0100},
author = {Menotti, Pietro},
biburl = {https://www.bibsonomy.org/bibtex/266c4efbcf91ee2e2bcf85239b7846670/jpschaar},
description = {On the semiclassical treatment of Hawking radiation},
interhash = {860afa481d6ffbb87ea5a379b1602b03},
intrahash = {66c4efbcf91ee2e2bcf85239b7846670},
keywords = {black hawking holes radiation},
note = {cite arxiv:0911.4358
Comment: 18 pages, LaTeX},
timestamp = {2009-11-27T10:52:35.000+0100},
title = {On the semiclassical treatment of Hawking radiation},
url = {http://arxiv.org/abs/0911.4358},
year = 2009
}