Supernova neutrino detection in NOvA
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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