Enviar artigo por via de e-mail Schwinger vs Unruh
- Autores: Volovik G.E1,2
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Afiliações:
- Low Temperature Laboratory, Aalto University
- Landau Institute for Theoretical Physics
- Edição: Volume 120, Nº 9-10 (2024)
- Páginas: 659-660
- Seção: 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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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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