Fabbri A, Navarro D J, Navarro-Salas J
Dipartimento di Fisica dell'Università di Bologna and INFN sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy.
Phys Rev Lett. 2000 Sep 18;85(12):2434-7. doi: 10.1103/PhysRevLett.85.2434.
The formation of near-extremal Reissner-Nordström black holes in the S-wave approximation can be described, near the event horizon, by an effective solvable model. The corresponding one-loop quantum theory remains solvable and allows one to follow analytically the evaporation process, which is shown to require an infinite amount of time.
在S波近似下，近极端雷斯纳 - 诺德斯特龙黑洞的形成在事件视界附近可以用一个有效的可解模型来描述。相应的单圈量子理论仍然是可解的，并且允许人们通过解析方法追踪蒸发过程，结果表明这需要无限长的时间。
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