Schwinger vs Unruh
Fuente:
arXiv
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| Autore principale: | |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| Soggetti: | |
| Accesso online: | |
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| _version_ | 1866917769386131456 |
|---|---|
| author | Volovik, G. E. |
| author_facet | Volovik, G. E. |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_03316 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Schwinger vs Unruh Volovik, G. E. General Relativity and Quantum Cosmology Other Condensed Matter High Energy Physics - Phenomenology 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. |
| title | Schwinger vs Unruh |
| topic | General Relativity and Quantum Cosmology Other Condensed Matter High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2409.03316 |