Supernova neutrino detection in NOvA

Acero, M A and Adamson, P. and Agam, G. and Giri, Anjan Kumar et. al. (2020) Supernova neutrino detection in NOvA. Journal of Cosmology and Astroparticle Physics, 2020 (10). 014. ISSN 1475-7516

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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.

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IITH Creators:
IITH CreatorsORCiD
Giri, Anjan KumarUNSPECIFIED
Item Type: Article
Uncontrolled Keywords: Core-collapse supernovae; Neutrino experiments; Supernova neutrinos
Subjects: Physics
Divisions: Department of Physics
Depositing User: . LibTrainee 2021
Date Deposited: 14 Jul 2021 06:03
Last Modified: 14 Jul 2021 06:03
URI: http://raiith.iith.ac.in/id/eprint/8306
Publisher URL:
OA policy: https://v2.sherpa.ac.uk/id/publication/11312
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