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Schwinger vs Unruh
- Authors: Volovik G.E1,2
-
Affiliations:
- Low Temperature Laboratory, Aalto University
- Landau Institute for Theoretical Physics
- Issue: Vol 120, No 9-10 (2024)
- Pages: 659-660
- Section: Articles
- URL: https://journal-vniispk.ru/0370-274X/article/view/271828
- DOI: https://doi.org/10.31857/S0370274X24110014
- EDN: https://elibrary.ru/PBFIOH
- ID: 271828
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Abstract
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.
About the authors
G. E Volovik
Low Temperature Laboratory, Aalto University; Landau Institute for Theoretical Physics
Author for correspondence.
Email: volovikgrigory@gmail.com
Aalto, Finland; Chernogolovka, Russia
References
- V. Akhmedova, T. Pilling, A. de Gill, and D. Singleton, Phys. Lett. B 673, 227 (2009).
- A. de Gill, Am. J. Phys. 78, 685 (2010).
- G.E. Volovik, Symmetry 16, 763 (2024).
- J. Schwinger, Phys. Rev. 82, 664 (1951).
- J. Schwinger, Phys. Rev. 93, 616 (1953).
- W.G. Unruh, Phys. Rev. D 14, 870 (1976).
- R. Parentani and S. Massar, Phys. Rev. D 55, 3603 (1997).
- D. Kharzeev and K. Tuchin, Nucl. Phys. A 753, 316 (2005).
- V. Sudhir, N. Stritzelberger, and A. Kempf, Phys. Rev. D 103, 105023 (2021).
- M. Teslyk, O. Teslyk, L. Zadorozhna, L. Bravina, and E. Zabrodin, Particles 5, 157 (2022).
- G.W. Gibbons and S.W. Hawking, Phys. Rev. D 15, 2738 (1977).
- G. ’t Hooft, Universe 8, 537 (2022).
- G. ’t Hooft, J. Phys.: Conf. Ser. 2533, 012015 (2023).
- G.E. Volovik, JETP Lett. 69, 705 (1999).
- M.K. Parikh and F. Wilczek, Phys. Rev. Lett. 85, 5042 (2000).
- J.D. Brown and J.W. York, Jr., Phys. Rev. D 47, 1407 (1993).
- S. Nojiri, S.D. Odintsov, and V. Faraoni, Phys. Rev. D 104, 084030 (2021).
- B. Reznik, Phys. Rev. B 57, 2403 (1998).
- R. Casadio and G. Venturi, Phys. Lett. A 252, 109 (1999).
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