| Near-extremal Black Hole |
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In Supersymmetric theories, near-extremal black holes are often small perturbations of supersymmetric black holes. Such black holes have a very small Hawking Temperature and consequently emit a small amount of Hawking Radiation . Their Black Hole Entropy can often be calculated in String Theory , much like in the case of extremal black holes, at least to the first order in non-extremality. |
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