The Hawking effect for a collapsing star in an initial state of KMS type

Physics

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Scientific paper

We prove the Hawking effect for gravitational collapse of a charged star in an expanding universe or not, stationary in the past and collapsing to a black hole in the future. In the past, the quantum initial state of the Dirac fields was given by a KMS state with unspecified temperature. With the same physical model, this paper generalizes our previous work to the case of a quantum initial state of KMS type rather than a Boulware vacuum.

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