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Title: Supernova neutrino detection in NOvA

Journal Article · · Journal of Cosmology and Astroparticle Physics
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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 $$\mathcal{O}(10~\text{MeV})$$. This signature provides a means to study the dominant mode of energy release for a core-collapse supernova occurring in our galaxy. In this paper, 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$$_\odot$$ to 27\~M$$_\odot$$, respectively.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); State of Minnesota
Contributing Organization:
NOvA Collaboration
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1633748
Report Number(s):
arXiv:2005.07155; FERMILAB-PUB-20-201-E; oai:inspirehep.net:1796383; TRN: US2201231
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2020, Issue 10; ISSN 1475-7516
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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