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The number of expected ν-induced background events for each energy bin (black -geo-¯ ν e , red -reactor ¯ ν e , green -atmospheric ν).

The number of expected ν-induced background events for each energy bin (black -geo-¯ ν e , red -reactor ¯ ν e , green -atmospheric ν).

Source publication
Preprint
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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...

Contexts in source publication

Context 1
... most relevant sources of ¯ ν e events below 10 MeV are the Earth's radioactive isotopes and the nuclear reactors, while at higher energies the atmospheric neutrino background dominates the energy spectrum (see Fig.1). In the following, we provide the details about each of these backgrounds. ...
Context 2
... of 0.1 MeV, from 3.5 to 5 MeV in increments of 0.5 MeV, and for E ν > 5 MeV in 1.0 MeV steps. In order to maximize the signal to background ratio, the lower integration limits T th from Eq. 29 was optimized for different neutrino energies considering the shape of the spectrum decreasing with energy (Fig. 7). The three blue lines indicated in Fig. 7 with indices 1, 2, and 3 show the thresholds of electron energies T th , for which E ν was set to (1.5, 3.5) MeV, (4.0, 5.0) MeV, and (6.0, 15.0) MeV intervals, ...
Context 3
... most relevant sources of ¯ ν e events below 10 MeV are the Earth's radioactive isotopes and the nuclear reactors, while at higher energies the atmospheric neutrino background dominates the energy spectrum (see Fig.1). In the following, we provide the details about each of these backgrounds. ...
Context 4
... of 0.1 MeV, from 3.5 to 5 MeV in increments of 0.5 MeV, and for E ν > 5 MeV in 1.0 MeV steps. In order to maximize the signal to background ratio, the lower integration limits T th from Eq. 29 was optimized for different neutrino energies considering the shape of the spectrum decreasing with energy (Fig. 7). The three blue lines indicated in Fig. 7 with indices 1, 2, and 3 show the thresholds of electron energies T th , for which E ν was set to (1.5, 3.5) MeV, (4.0, 5.0) MeV, and (6.0, 15.0) MeV intervals, ...

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