On-line recognition of supernova neutrino bursts in the LVD

• Published in: Astroparticle physics Vol. 28; no. 6; pp. 516 - 522
• Main Authors: Agafonova, N.Yu, Aglietta, M., Antonioli, P., Bari, G., Bonardi, A., Boyarkin, V.V., Bruno, G., Fulgione, W., Galeotti, P., Garbini, M., Ghia, P.L., Giusti, P., Gomez, F., Kemp, E., Kuznetsov, V.V., Kuznetsov, V.A., Malguin, A.S., Menghetti, H., Pesci, A., Persiani, R., Pless, I.A., Porta, A., Ryasny, V.G., Ryazhskaya, O.G., Saavedra, O., Sartorelli, G., Selvi, M., Vigorito, C., Votano, L., Yakushev, V.F., Zatsepin, G.T., Zichichi, A.
• Format: Journal Article
• Language: English
• Published: Elsevier B.V 2008; Elsevier
• Subjects: Burst identification; LVD; Neutrino detection; Physics; Supernova core collapse; Neutrino detection; 97.60.Bw; 29.40.Mc; 13.15.+g; LVD; Supernova core collapse; Burst identification; 95.55.Vj
• ISSN: 0927-6505; 1873-2852
• DOI: 10.1016/j.astropartphys.2007.09.005

In this paper we show the capabilities of the Large Volume Detector (INFN Gran Sasso National Laboratory) to identify a neutrino burst associated with a supernova explosion, in the absence of an “external trigger”, e.g., an optical observation. We describe how the detector trigger and event selection have been optimized for this purpose, and we detail the algorithm used for the on-line burst recognition. The on-line sensitivity of the detector is defined and discussed in terms of supernova distance and ν ¯ e intensity at the source.