On the Quantum Levels of Isolated Spherically Symmetric Gravitational Systems
نویسنده
چکیده
The known canonical quantum theory of a spherically symmetric pure (Schwarzschild) gravitational system describes isolated black holes by plane waves exp(−iMc2τ/h̄) with respect to their continuous masses M and the proper time τ of observers at spatial infinity. On the other hand Bekenstein and Mukhanov postulated discrete mass levels for such black holes in the spirit of the Bohr-Sommerfeld quantisation in atomic physics. The two approaches can be related by postulating periodic boundary conditions in time for the plane waves and by identifying the period ∆ in real time E-Mail: [email protected]
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تاریخ انتشار 1996