prikaz prve stranice dokumenta Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
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Scientific paper - Original scientific paper
Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
Symmetry, 15 (2023), 11; 1970. https://doi.org/10.3390/sym15111970
Dadić, Ivan; Klabučar, Dubravko

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Dadić, I. & Klabučar, D. (2023). Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory. Symmetry, 15. (11). doi: 10.3390/sym15111970

Dadić, Ivan and Dubravko Klabučar. "Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory." Symmetry, vol. 15, no. 11, 2023. https://doi.org/10.3390/sym15111970

Dadić, Ivan and Dubravko Klabučar. "Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory." Symmetry 15, no. 11 (2023). https://doi.org/10.3390/sym15111970

Dadić, I. and Klabučar, D. (2023) 'Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory', Symmetry, 15(11). doi: 10.3390/sym15111970

Dadić I, Klabučar D. Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory. Symmetry [Internet]. 2023 October 24 [cited 2024 October 07];15(11). doi: 10.3390/sym15111970

I. Dadić and D. Klabučar, "Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory", Symmetry, vol. 15, no. 11, October 2023. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:596605. [Accessed: 07 October 2024]

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Metadata
Title (english)Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
AuthorIvan Dadić
AuthorDubravko Klabučar
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
We demonstrate that the Finite-Time-Path Field Theory is an adequate tool for calculating neutrino oscillations. We apply this theory using a mass-mixing Lagrangian which involves the correct Dirac spin and chirality structure and a Pontecorvo–Maki–Nakagawa–Sakata (PMNS)-like mixing matrix. The model is exactly solvable. The Dyson–Schwinger equations transform propagators of the input free (massless) flavor neutrinos into a linear combination of oscillating (massive) neutrinos. The results are consistent with the predictions of the PMNS matrix while allowing for extrapolation to early times.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleSymmetry
Numberingvol. 15, no. 11, 1970
e-ISSN2073-8994
DOIhttps://doi.org/10.3390/sym15111970
URN:NBNurn:nbn:hr:217:596605
Publication2023-10-24
Document URLhttps://www.mdpi.com/2073-8994/15/11/1970
Type of resourceText
Access conditionsOpen access
Terms of useLicence Attribution 4.0 International (CC BY 4.0) icon
Public note© 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Received: 3 July 2023. Revised: 11 September 2023. Accepted: 21 September 2023. Published: 24 October 2023.
Created on2024-07-19 12:31:46