Quantization of the Reissner-Nordstr\"{o}m Black Hole
Quantization of the Reissner-Nordstr\"{o}m Black Hole
The Reissner--Nordstr\"{o}m family of solutions can be understood to arise from the spherically symmetric sector of a nonlinear SO(2,1)/SO(1,1) sigma model coupled to three dimensional Euclidean gravity. In this context a group theoretical quantization is performed. We identify the observables of the theory and calculate their spectra.
D. Maison、H. Hollmann、P. Breitenlohner
Munich, Max Planck Inst.Cambridge, DAMTPMunich, Max Planck Inst.
物理学
D. Maison,H. Hollmann,P. Breitenlohner.Quantization of the Reissner-Nordstr\"{o}m Black Hole[EB/OL].(1998-04-10)[2025-08-02].https://arxiv.org/abs/gr-qc/9804030.点此复制
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