The Wave Function of a Collapsing Star and Quantization Conditions

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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13 pages, BRX-TH-342

Scientific paper

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.

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