Hawking temperature for a large class of black holes (Schwarzschild, Reissner–Nordström, (Anti) de Sitter, with spherical, toroidal and hyperboloidal topologies) is computed using only laws of classical physics plus the “classical” Heisenberg Uncertainty Principle. This principle is shown to be fully sufficient to get the result, and there is no need to this scope of a Generalized Uncertainty Principle or an Extended Uncertainty Principle.

中文翻译：

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海森堡测不准原理对各种黑洞的霍金温度

仅使用经典物理定律和“经典”海森堡不确定性原理来计算一大类黑洞（Schwarzschild、Reissner–Nordström、(Anti) de Sitter，具有球形、环形和双曲面拓扑）的霍金温度。这个原则被证明是完全足以得到结果的，并且不需要广义不确定性原则或扩展不确定性原则的这个范围。