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arXiv · hep-ph/0012082

Supernova Neutrino Detection in Borexino

L. Cadonati·F. P. Calaprice·M. C. Chen
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Abstract

We calculated the expected neutrino signal in Borexino from a typical Type II supernova at a distance of 10 kpc. A burst of around 110 events would appear in Borexino within a time interval of about 10 s. Most of these events would come from the reaction channel $\barν_e+p\to e^++n$, while about 30 events would be induced by the interaction of the supernova neutrino flux on $^{12}$C in the liquid scintillator. Borexino can clearly distinguish between the neutral-current excitations $^{12}{C}(ν,ν')^{12}{C}^*$(15.11 MeV) and the charged-current reactions $^{12}{C}(ν_e,e^-)^{12}{N}$ and $^{12}{C}(\barν_e,e^+)^{12}{B}$, via their distinctive event signatures. The ratio of the charged-current to neutral-current neutrino event rates and their time profiles with respect to each other can provide a handle on supernova and non-standard neutrino physics (mass and flavor oscillations).

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L. Cadonati, F. P. Calaprice, M. C. Chen. 2000-12-07. Supernova Neutrino Detection in Borexino. https://doi.org/10.1016/s0927-6505(01)00129-3

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