Supernova neutrino detection in NOvA

0537595 - FZÚ 2021 RIV GB eng J - Článek v odborném periodiku
Acero, M. A. - Adamson, P. - Agam, G. - Filip, Peter - Hakl, František - Lokajíček, Miloš - Zálešák, Jaroslav … celkem 201 autorů
Supernova neutrino detection in NOvA.
Journal of Cosmology and Astroparticle Physics. Roč. 2020, č. 10 (2020), s. 1-34, č. článku 014. ISSN 1475-7516. E-ISSN 1475-7516
Výzkumná infrastruktura: Fermilab-CZ II - 90113
Institucionální podpora: RVO:68378271 ; RVO:67985807
Klíčová slova: NOvA * neutrino * supernova * calorimeter * scintillation counter * liquid * trigger
Obor OECD: Particles and field physics; Particles and field physics (UIVT-O)
Impakt faktor: 5.839, rok: 2020
Způsob publikování: Omezený přístup
https://doi.org/10.1088/1475-7516/2020/10/014

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 &calO,(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 supernova from progenitor stars with masses of 9.6 M⊙ to 27 M⊙, respectively.

Trvalý link: http://hdl.handle.net/11104/0315417