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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Published in | Astroparticle physics Vol. 28; no. 6; pp. 516 - 522 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
2008
Elsevier |
Subjects | |
Online Access | Get full text |
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Abstract | 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. |
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AbstractList | 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. In this paper we show the capabilities of the Large Volume Detector (INFN GranSasso National Laboratory) to identify a neutrino burst associated to a supernovaexplosion, in the absence of an ”external trigger”, e.g., an optical observation. Wedescribe how the detector trigger and event selection have been optimized for thispurpose, and we detail the algorithm used for the on-line burst recognition. Theon-line sensitivity of the detector is defined and discussed in terms of supernovadistance and ¯νe intensity at the source. |
Author | Menghetti, H. Malguin, A.S. Garbini, M. Boyarkin, V.V. Bruno, G. Porta, A. Sartorelli, G. Antonioli, P. Kuznetsov, V.A. Yakushev, V.F. Ghia, P.L. Ryasny, V.G. Pesci, A. Bonardi, A. Kemp, E. Fulgione, W. Ryazhskaya, O.G. Kuznetsov, V.V. Votano, L. Persiani, R. Vigorito, C. Agafonova, N.Yu Aglietta, M. Pless, I.A. Zatsepin, G.T. Giusti, P. Galeotti, P. Saavedra, O. Selvi, M. Zichichi, A. Bari, G. Gomez, F. |
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67010 Assergi LAquila, Italy – sequence: 23 givenname: V.G. surname: Ryasny fullname: Ryasny, V.G. organization: Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia – sequence: 24 givenname: O.G. surname: Ryazhskaya fullname: Ryazhskaya, O.G. organization: Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia – sequence: 25 givenname: O. surname: Saavedra fullname: Saavedra, O. organization: Institute of Physics of Interplanetary Space, INAF, Torino, University of Torino and INFN-Torino, c/o Laboratori Nazionali del Gran Sasso, S.S. 17 BIS km. 18.910, 67010 Assergi LAquila, Italy – sequence: 26 givenname: G. surname: Sartorelli fullname: Sartorelli, G. organization: University of Bologna and INFN-Bologna, Italy – sequence: 27 givenname: M. surname: Selvi fullname: Selvi, M. organization: University of Bologna and INFN-Bologna, Italy – sequence: 28 givenname: C. surname: Vigorito fullname: Vigorito, C. organization: Institute of Physics of Interplanetary Space, INAF, Torino, University of Torino and INFN-Torino, c/o Laboratori Nazionali del Gran Sasso, S.S. 17 BIS km. 18.910, 67010 Assergi LAquila, Italy – sequence: 29 givenname: L. surname: Votano fullname: Votano, L. organization: INFN-LNF, Frascati, Italy – sequence: 30 givenname: V.F. surname: Yakushev fullname: Yakushev, V.F. organization: Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia – sequence: 31 givenname: G.T. surname: Zatsepin fullname: Zatsepin, G.T. organization: Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia – sequence: 32 givenname: A. surname: Zichichi fullname: Zichichi, A. organization: University of Bologna and INFN-Bologna, Italy |
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Keywords | Neutrino detection 97.60.Bw 29.40.Mc 13.15.+g LVD Supernova core collapse Burst identification 95.55.Vj |
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References | Agafonova (bib6) 2007; 27 Antonioli (bib11) 2004; 6 Alekseev, Alekseeva, Volchenko, Krivosheina, Alekseev, Alekseeva, Volchenko, Krivosheina (bib3) 1987; 45 Jegerlehner, Neubig, Raffelt (bib13) 1996; 54 Bigongiari, Fulgione, Passuello, Saavedra, Trinchero (bib7) 1990; 288 Keil, Raffelt, Janka (bib16) 2003; 590 Strumia, Vissani (bib12) 2005; 726 Costantini, Ianni, Pagliaroli, Vissani (bib15) 2007; 05 Antonioli, Fulgione, Galeotti, Panaro (bib9) 1991; 309 N.Yu. Agafonova et al., LNGS/EXP-01/07, EPJ C, accepted for publication. Aglietta, Dadykin (bib4) 1987; 3 Hirata, Hirata (bib1) 1987; 58 Aglietta (bib5) 1992; 105 Costantini, Ianni, Vissani (bib14) 2004; 70 Bionta (bib2) 1987; 58 A. Porta, Ph.D. Thesis, University of Torino, 2005. |
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Snippet | 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... In this paper we show the capabilities of the Large Volume Detector (INFN GranSasso National Laboratory) to identify a neutrino burst associated to a... |
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SubjectTerms | Burst identification LVD Neutrino detection Physics Supernova core collapse |
Title | On-line recognition of supernova neutrino bursts in the LVD |
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