Supernova neutrino detection in NOvA
Creators: name: NOvA Collaboration
name: Acero, M. A.
name: Adamson, P.
name: Agam, G.
name: Aliaga, L.
name: Alion, T.
name: Allakhverdian, V.
name: Anfimov, N.
name: Antoshkin, A.
name: Arrieta-Diaz, E.
name: Asquith, L.
name: Aurisano, A.
name: Back, A.
name: Backhouse, C.
name: Baird, M.
name: Balashov, N.
name: Baldi, P.
name: Bambah, B. A.
name: Bashar, S.
name: Bays, K.
name: Bending, S.
name: Bernstein, R.
name: Bhatnagar, V.
name: Bhuyan, B.
name: Bian, J.
name: Blair, J.
name: Booth, A. C.
name: Bour, P.
name: Bowles, R.
name: Bromberg, C.
name: Buchanan, N.
name: Butkevich, A.
name: Bychkov, V.
name: Calvez, S.
name: Carroll, T. J.
name: Catano-Mur, E.
name: Childress, S.
name: Choudhary, B. C.
name: Coan, T. E.
name: Colo, M.
name: Corwin, L.
name: Cremonesi, L.
name: Davies, G. S.
name: Derwent, P. F.
name: Ding, P.
name: Djurcic, Z.
name: Dolce, M.
name: Doyle, D.
name: Tonguino, D. Dueñas
name: Dukes, E. C.
name: Dung, P.
name: Duyang, H.
name: Edayath, S.
name: Ehrlich, R.
name: Elkins, M.
name: Feldman, G. J.
name: Filip, P.
name: Flanagan, W.
name: Franc, J.
name: Frank, M. J.
name: Gallagher, H. R.
name: Gandrajula, R.
name: Gao, F.
name: Germani, S.
name: Giri, A.
name: Gomes, R. A.
name: Goodman, M. C.
name: Grichine, V.
name: Groh, M.
name: Group, R.
name: Guo, B.
name: Habig, A.
name: Hakl, F.
name: Hall, A.
name: Hartnell, J.
name: Hatcher, R.
name: Hatzikoutelis, A.
name: Heller, K.
name: Hewes, V
name: Himmel, A.
name: Holin, A.
name: Howard, B.
name: Huang, J.
name: Hylen, J.
name: Jediny, F.
name: Johnson, C.
name: Judah, M.
name: Kakorin, I.
name: Kalra, D.
name: Kaplan, D. M.
name: Keloth, R.
name: Klimov, O.
name: Koerner, L. W.
name: Kolupaeva, L.
name: Kotelnikov, S.
name: Kubu, M.
name: Kullenberg, Ch.
name: Kumar, A.
name: Kuruppu, C. D.
name: Kus, V.
name: Lackey, T.
name: Lang, K.
name: Li, L.
name: Lin, S.
name: Lister, A.
name: Lokajicek, M.
name: Luchuk, S.
name: Magill, S.
name: Mann, W. A.
name: Marshak, M. L.
name: Martinez-Casales, M.
name: Matveev, V.
name: Mayes, B.
name: Méndez, D. P.
name: Messier, M. D.
name: Meyer, H.
name: Miao, T.
name: Miller, W. H.
name: Mishra, S. R.
name: Mislivec, A.
name: Mohanta, R.
name: Moren, A.
name: Morozova, A.
name: Mualem, L.
name: Muether, M.
name: Mufson, S.
name: Mulder, K.
name: Murphy, R.
name: Musser, J.
name: Naples, D.
name: Nayak, N.
name: Nelson, J. K.
name: Nichol, R.
name: Nikseresht, G.
name: Niner, E.
name: Norman, A.
name: Norrick, A.
name: Nosek, T.
name: Olshevskiy, A.
name: Olson, T.
name: Paley, J.
name: Patterson, R. B.
name: Pawloski, G.
name: Petrova, O.
name: Petti, R.
name: Plunkett, R. K.
name: Psihas, F.
name: Rafique, A.
name: Raj, V.
name: Ramson, B.
name: Rebel, B.
name: Rojas, P.
name: Ryabov, V.
name: Samoylov, O.
name: Sanchez, M. C.
name: Falero, S. Sánchez
name: Seong, I. S.
name: Shanahan, P.
name: Sheshukov, A.
name: Singh, P.
name: Singh, V.
name: Smith, E.
name: Smolik, J.
name: Snopok, P.
name: Solomey, N.
name: Sousa, A.
name: Soustruznik, K.
name: Strait, M.
name: Suter, L.
name: Sutton, A.
name: Sweeney, C.
name: Talaga, R. L.
name: Oregui, B. Tapia
name: Tas, P.
name: Thayyullathil, R. B.
name: Thomas, J.
name: Tiras, E.
name: Torbunov, D.
name: Tripathi, J.
name: Tsaris, A.
name: Torun, Y.
name: Urheim, J.
name: Vahle, P.
name: Vallari, Z.
name: Vasel, J.
name: Vokac, P.
name: Vrba, T.
name: Wallbank, M.
name: Warburton, T. K.
name: Wetstein, M.
name: Whittington, D.
name: Wickremasinghe, D. A.
name: Wojcicki, S. G.
name: Wolcott, J.
name: Dombara, A. Yallappa
name: Yonehara, K.
name: Yu, S.
name: Yu, Y.
name: Zadorozhnyy, S.
name: Zalesak, J.
name: Zhang, Y.
name: Zwaska, R.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: 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. 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 9.6M$_\odot$ to 27M$_\odot$, respectively.
description: 30 pages, 17 figures