Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model
Meng-Ru Wu, Yong-Zhong Qian, Gabriel Martinez-Pinedo, Tobias Fischer,, Lutz Huther

TL;DR
This study investigates how neutrino flavor oscillations influence supernova nucleosynthesis and neutrino detection, revealing their impact on isotope production and potential to determine neutrino mass hierarchy.
Contribution
It provides detailed analysis of collective neutrino oscillations' effects on nucleosynthesis and neutrino signals using a realistic supernova model, highlighting the sensitivity to spectral and density evolution.
Findings
Oscillations enhance production of 138La and 180Ta
Little impact on nu p-process nucleosynthesis
Potential to infer neutrino mass hierarchy from detector signals
Abstract
In this paper, we explore the effects of neutrino flavor oscillations on supernova nucleosynthesis and on the neutrino signals. Our study is based on detailed information about the neutrino spectra and their time evolution from a spherically-symmetric supernova model for an 18 M progenitor. We find that collective neutrino oscillations are not only sensitive to the detailed neutrino energy and angular distributions at emission, but also to the time evolution of both the neutrino spectra and the electron density profile. We apply the results of neutrino oscillations to study the impact on supernova nucleosynthesis and on the neutrino signals from a Galactic supernova. We show that in our supernova model, collective neutrino oscillations enhance the production of rare isotopes 138La and 180Ta but have little impact on the nu p-process nucleosynthesis. In addition, the adiabatic MSW flavor…
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