Journals / Turkish Journal of Physics / 2018 / Cilt: 42 - Sayı: 5

An analytic solution to the spin flavor precession for solar Majorana neutrinos in the case of three neutrino generations

Pages
600–612
Publication Date
2022-11-04
DOI
—
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AI Summary & Key Takeaways

AI Insight
⚡ TL;DR(Too Long; Didn't Read)

The accuracyof the formulas is checked for two different magnetic field profiles in the Sun.

📌 3 Key Takeaways

🎯
Objective & Hypothesis:The spin flavor precession (SFP) is investigated in the three neutrino generation case assuming that theneutrinos are of Majorana type.
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Key Findings & Data:Approximate analytical formulas including all transition magnetic moments are providedfor the electron neutrino survival probability and νe → νe transition probability in the SFP framework.
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Conclusion & Impact:The accuracyof the formulas is checked for two different magnetic field profiles in the Sun.
🔬Design:Research Article
📍Scope:Comprehensive Sample
⚙️Variables:Domain Parameters

Abstract

The spin flavor precession (SFP) is investigated in the three neutrino generation case assuming that theneutrinos are of Majorana type. Approximate analytical formulas including all transition magnetic moments are providedfor the electron neutrino survival probability and νe → νe transition probability in the SFP framework. The accuracyof the formulas is checked for two different magnetic field profiles in the Sun.

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Cite This Article

YILMAZ, D. (2022). An analytic solution to the spin flavor precession for solar Majorana neutrinos in the case of three neutrino generations. Turkish Journal of Physics, Cilt: 42 - Sayı: 5, 600–612. https://ajindex.com/articles/613995

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