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Killing horizons kill horizon degrees

机译:杀死地平线杀死地平线

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摘要

Frequently, it is argued that the microstates responsible for the Bekenstein-Hawking entropy should arise from some physical degrees of freedom located near or on the black hole horizon. In this essay, we elucidate that instead entropy may emerge from the conversion of physical degrees of freedom, attached to a generic boundary, into unobservable gauge degrees of freedom attached to the horizon. By constructing the reduced phase space, it can be demonstrated that such a transmutation indeed takes place for a large class of black holes, including Schwarzschild.
机译:通常,人们认为,引起Bekenstein-Hawking熵的微观状态应该来自位于黑洞视界附近或之上的某些物理自由度。在本文中,我们阐明了熵可能会从附着在通用边界上的物理自由度转换为附着在地平线上的不可观测的标度自由度而出现。通过构造减少的相空间,可以证明这种变换确实发生在包括Schwarzschild在内的大类黑洞中。

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