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Expected fluxes for the DSNB ¯ ν e predicted by Nakazato et al. [52] (red) and Hudepohl et al. [53] (black) models.

Expected fluxes for the DSNB ¯ ν e predicted by Nakazato et al. [52] (red) and Hudepohl et al. [53] (black) models.

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Figure 1: The number of expected ν-induced background events for each...
Figure 2: Reactor antineutrino spectra expected in Borexino, assuming...
Figure 3: The number of measured events (black data point) is compared...
Figure 4: New Borexino model-independent limits on electron ¯ ν e...
+4 Figure 5: Expected fluxes for the DSNB ¯ ν e predicted by Nakazato et...
Search for low-energy neutrinos from astrophysical sources with Borexino
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  • Sep 2019
We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent uppe...
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Context 1
... expected DSNB fluxes at the detector for both models are reported in Fig. ...
Context 2
... expected DSNB fluxes at the detector for both models are reported in Fig. ...

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