``Cosmological'' vacuum state for a black hole immersed in an expanding Friedmann universe

Mathematics – Logic

Scientific paper

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Scientific paper

The quantization in a ``vacuum'' state defined by cosmological boundary
conditions is discussed for a massless scalar field propagating on a
two-dimensional Schwarzschild space-time. The expectation values of the
stress tensor in this state are found to be regular both on the future
and past horizons.

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