The Wave Function of a Collapsing Star and Quantization Conditions
High Energy Physics - Theory
2007-05-23 v1
Abstract
A very simple minisuperspace describing the Oppenheimer-Snyder collapsing star is found. The semiclasical wave function of that model turn out to describe a bound state. For fixed initial radius of the collapsing star, the corrssponding Bohr-Sommerfeld quantization condition implies mass quantization. An extension of this model, and some consequences, are considered.
Cite
@article{arxiv.hep-th/9303169,
title = {The Wave Function of a Collapsing Star and Quantization Conditions},
author = {Yoav Peleg},
journal= {arXiv preprint arXiv:hep-th/9303169},
year = {2007}
}
Comments
13 pages, BRX-TH-342