A Kerr black hole at the zero temperature limit continues to radiate in modes with frequency below mΩ, peaking at ω=mΩ/2.
Zel’dovich, JETP 35, 1085 (1972)
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Hawking radiation at the zero temperature limit
A Kerr black hole at the zero temperature limit continues to radiate in modes with frequency below mΩ, peaking at ω=mΩ/2.