Schwinger vs Unruh

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Resumo

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.

Sobre autores

G. Volovik

Low Temperature Laboratory, Aalto University; Landau Institute for Theoretical Physics

Autor responsável pela correspondência
Email: volovikgrigory@gmail.com
Aalto, Finland; Chernogolovka, Russia

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