The Wave Function of a Collapsing Star and Quantization Conditions

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dc.creatorPeleg, Yoav
dc.date1993-03-30
dc.date.accessioned2026-07-07T04:19:21Z
dc.date.available2026-07-07T04:19:21Z
dc.descriptionA 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.
dc.description13 pages, BRX-TH-342
dc.identifierhttps://arxiv.org/abs/hep-th/9303169
dc.identifierhttp://arxiv.org/abs/hep-th/9303169
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53516
dc.subjectHigh Energy Physics - Theory
dc.titleThe Wave Function of a Collapsing Star and Quantization Conditions
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