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On-line recognition of supernova neutrino bursts in the LVD

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 selectio...

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Bibliographic Details
Published in:Astroparticle physics 2008, Vol.28 (6), p.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: Article
Language:English
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Summary: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.
ISSN:0927-6505
1873-2852
DOI:10.1016/j.astropartphys.2007.09.005