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Supernova neutrino detection in NOvA

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. Green open access

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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
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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