Schwinger vs Unruh

G. E. Volovik

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arXiv · 2409.03316

Schwinger vs Unruh

G. E. Volovik

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Abstract

It is shown that the temperatures which characterise the Unruh effect, the Gibbons-Hawking radiation from the de Sitter cosmological horizon and the Hawking radiation from the black hole horizon acquire the extra factor 2 compared with their traditional values. The reason for that is the coherence of different processes. The combination of the coherent processes also allows us to make the connection between the Schwinger pair production and the Unruh effect.

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BibTeX RIS

G. E. Volovik. 2024-09-05. Schwinger vs Unruh. https://arxiv.org/abs/2409.03316

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