Schwinger vs Unruh

Мұқаба

Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

G. Volovik

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

Хат алмасуға жауапты Автор.
Email: volovikgrigory@gmail.com
Aalto, Finland; Chernogolovka, Russia

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