Hawking radiation in an inflationary universe

Physics

Scientific paper

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Scientific paper

Abstract

We construct a spacetime which models the ``rolling phase'' of a Linde-Guth scenario. Although the spacetime has neither the special symmetries, nor the event horizons, of de Sitter space, we show it does have de Sitter-like Hawking radiation. This Hawking temperature necessitates modifying the use of the finite temperature effective potential in the proposed scenarios.

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