prikaz prve stranice dokumenta Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
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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

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Dadić, I. 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 i Dubravko Klabučar. "Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory." Symmetry, vol. 15, br. 11, 2023. https://doi.org/10.3390/sym15111970

Dadić, Ivan i Dubravko Klabučar. "Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory." Symmetry 15, br. 11 (2023). https://doi.org/10.3390/sym15111970

Dadić, I. i 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]. 24.10.2023. [pristupljeno 24.08.2024.];15(11). doi: 10.3390/sym15111970

I. Dadić i D. Klabučar, "Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory", Symmetry, vol. 15, br. 11, Listopad 2023. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:596605. [Citirano: 24.08.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:596605
Podaci o radu
Naslov (engleski)Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory
AutorIvan Dadić
AutorDubravko Klabučar
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
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.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaSymmetry
Brojčani podacivol. 15, br. 11, 1970
e-ISSN2073-8994
DOIhttps://doi.org/10.3390/sym15111970
URN:NBNurn:nbn:hr:217:596605
Datum objave publikacije2023-10-24
URL dokumentahttps://www.mdpi.com/2073-8994/15/11/1970
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Imenovanje 4.0 međunarodna (CC BY 4.0)
Javna napomena© 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.
Datum i vrijeme pohrane2024-07-19 12:31:46