Acero, MA;
Adamson, P;
Agam, G;
Aliaga, L;
Alion, T;
Allakhverdian, V;
Anfimov, N;
... et alia, .; + view all
(2020)
Supernova neutrino detection in NOvA.
Journal of Cosmology and Astroparticle Physics
, 2020
(10)
, Article 14. 10.1088/1475-7516/2020/10/014.
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Abstract
The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse supernova through inverse beta decay interactions on carbon at energies of O(10 MeV). This signature provides a means to study the dominant mode of energy release for a core-collapse supernova occurring in our galaxy. We describe the data-driven software trigger system developed and employed by the NOvA experiment to identify and record neutrino data from nearby galactic supernovae. This technique has been used by NOvA to self-trigger on potential core-collapse supernovae in our galaxy, with an estimated sensitivity reaching out to 10 kpc distance while achieving a detection efficiency of 23% to 49% for supernovae from progenitor stars with masses of 9.6 M☉ to 27 M☉, respectively.
Type: | Article |
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Title: | Supernova neutrino detection in NOvA |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1088/1475-7516/2020/10/014 |
Publisher version: | https://doi.org/10.1088/1475-7516/2020/10/014 |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions. |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10116055 |
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