Resonant Spin-Flavor Conversion of Supernova Neutrinos: Dependence on Electron Mole Fraction
T. Yoshida (1), A. Takamura (2), K. Kimura (3), H. Yokomakura (3), S., Kawagoe (1), T. Kajino (4) ((1) Univ. of Tokyo, (2) Toyota Coll. Tech.,, (3)Nagoya Univ., (4) NAOJ)

TL;DR
This paper investigates how the electron mole fraction in supernova environments influences resonant spin-flavor neutrino conversions, affecting observable neutrino spectra and event ratios, which can reveal neutrino properties and supernova conditions.
Contribution
It provides a detailed analysis of the dependence of RSF neutrino conversion on electron mole fraction and explores observable signatures in supernova neutrino detection.
Findings
Flavor conversion depends on Ye and mass hierarchy.
Event ratio variations can indicate RSF effects.
Time-dependent signatures help probe supernova conditions.
Abstract
Detailed dependence of resonant spin-flavor (RSF) conversion of supernova neutrinos on electron mole fraction Ye is investigated. Supernova explosion forms a hot-bubble and neutrino-driven wind region of which electron mole fraction exceeds 0.5 in several seconds after the core collapse. When a higher resonance of the RSF conversion is located in the innermost region, flavor change of the neutrinos strongly depends on the sign of 1-2Ye. At an adiabatic high RSF resonance the flavor conversion of bar{nu}_e -> nu_{mu,tau} occurs in Ye < 0.5 and normal mass hierarchy or in Ye > 0.5 and inverted mass hierarchy. In other cases of Ye values and mass hierarchies, the conversion of nu_e -> bar{nu}_{mu,tau} occurs. The final bar{nu}_e spectrum is evaluated in the cases of Ye < 0.5 and Ye > 0.5 taking account of the RSF conversion. Based on the obtained result, time variation of the event number…
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