Equivalence of Hawking and Unruh Temperatures and Entropies Through Flat Space Embeddings

Details Equivalence of Hawking and Unruh Temperatures and Entropies Through Flat Space Embeddings Equivalence of Hawking and Unruh Temperatures and Entropies Through Flat Space Embeddings

1998-06-27

arxiv.org/abs/hep-th/9806223v2

Class.Quant.Grav.15:L85-L87,1998

Physics

High Energy Physics

High Energy Physics - Theory

An expanded version of our initial submission: addition of entropy derivations to complement those of temperature in the origi

Scientific paper

10.1088/0264-9381/15/12/002

We present a unified description of temperature and entropy in spaces with either "true" or "accelerated observer" horizons: In their (higher dimensional) global embedding Minkowski geometries, the relevant detectors have constant accelerations a_{G}; associated with their Rindler horizons are temperature a_{G}/2\pi and entropy equal to 1/4 the horizon area. Both quantities agree with those calculated in the original curved spaces. As one example of this equivalence, we obtain the temperature and entropy of Schwarzschild geometry from its flat D=6 embedding.

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