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The third law of black hole thermodynamics: Quantum versus classical considerations
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-theory
Kehle and Unger have recently shown that, under suitable conditions, a massless charged classical scalar field can produce an extremal black hole in finite time. This result appears to violate the third law of thermodynamics (TLT), since extremal black holes have zero temperature. However, because t
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