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Quantum collapse of Newtonian dust shells*

M P Ryan Jr

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This paper considers a Newtonian approach to the quantum collapse of infinitesimally thin dust shells. It is possible to use elementary Newtonian calculations to find the equations of motion of the shell in terms of variables defined on the shell. The quantum problem reduces to the analogue of the non-relativistic hydrogen atom. One can study the Newtonian analogue of horizon formation by defining a 'horizon' as the point where the escape velocity at the surface of the shell becomes the speed of light. Various definitions of horizon formation in the quantum case will be considered.


Footnote
*  It is a great pleasure to be able to contribute to this special issue in honour of Vincent Moncrief. I have known Vince since we were graduate students together and have always admired his physical insight and capacity to solve complex problems with ease. I wish him many more productive years and even more success.
PACS

04.25.-g Approximation methods; equations of motion

04.60.Kz Lower dimensional models; minisuperspace models

04.20.Fy Canonical formalism, Lagrangians, and variational principles

04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics

MSC

83C57 Black holes

83C10 Equations of motion

83C45 Quantization of the gravitational field

Subjects

Gravitation and cosmology

Dates

Issue 3 (7 February 2004)

Received 30 October 2003

Published 13 January 2004



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