Мақаланы E-mail арқылы жіберу Schwinger vs Unruh
- Авторлар: Volovik G.E1,2
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Мекемелер:
- Low Temperature Laboratory, Aalto University
- Landau Institute for Theoretical Physics
- Шығарылым: Том 120, № 9-10 (2024)
- Беттер: 659-660
- Бөлім: Articles
- URL: https://cardiosomatics.ru/0370-274X/article/view/664460
- DOI: https://doi.org/10.31857/S0370274X24110014
- EDN: https://elibrary.ru/PBFIOH
- ID: 664460
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Рұқсат берілді
Рұқсат ақылы немесе 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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