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With a RN black hole, at fixed Q and sufficiently large R, the linear regime does not appear to extend all the way to saturation.
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With a RN black hole, at fixed Q and sufficiently large R, the linear regime does not appear to extend all the way to saturation.
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The discontinuous saturation for a strip and for a sphere in d = 3 for a RN black hole with a sufficiently large Q was first observed in [4]; see also Ref. [5].
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The discontinuous saturation for a strip and for a sphere in d = 3 for a RN black hole with a sufficiently large Q was first observed in [4]; see also Ref. [5].
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The expression below may not apply in d = 3, where we do not yet have a clean result.
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The expression below may not apply in d = 3, where we do not yet have a clean result.
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