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We consider quantum backreaction of the quantized scalar field with an arbitrary mass and curvature coupling on ultraextremal horizons. The problem is distinguished in that (in contrast to non-extremal or extremal black holes) the WKB approximation remains valid near (which is the radius of the horizon) even in the massless limit. We examine the behavior of the stress-energy tensor of the quantized field near and show that quantum-corrected objects under discussion do exist. In the limit of the large mass our results agree with previous ones known in literature.

生成讲解博客的中文版本

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