The Wave Function of a Collapsing Star and Quantization Conditions
نویسنده
چکیده
A very simple minisuperspace describing the Oppenheimer-Snyder collapsing star is found. The semiclassical wave function of that model turn out to describe a bound state. For fixed initial radius of the collapsing star, the corresponding Bohr-Sommerfeld quantization condition implies mass quantization. An extension of this model, and some consequences, are considered. This work is supported by the Fishbach Fellowship 92/3 and by the NSF grant PHY 88-04561.
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تاریخ انتشار 1993