The most powerful scintillator supernovae detector: LVD

M. Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Anzivino; G. Badino; Y. Ban; G. Bari; M. Basile; A. Benelli; V. S. Berezinsky; L. Bergamasco; S. Bianco; A. Bizzetti; G. Bruni; Y. Cao; G. Cara Romeo; R. Casaccia; C. Castagnoli; A. Castellina; K. Chen; R. Chen; J. A. Chinellato; L. Cifarelli; G. Cini; S. Cong; A. Contin; V. L. Dadikin; M. Dardo; A. De Silva; M. Deutsch; L. G. Dos Santos; R. I. Enikeev; F. L. Fabbri; W. Fulgione; P. Galeotti; P. L. Ghia; P. Giusti; F. Grianti; S. Gu; E. S. Hafen; P. Haridas; G. Iacobucci; N. Inoue; F. F. Khalchukov; E. V. Korolkova; P. V. Kortchaguin; V. B. Kortchaguin; V. A. Kudryavtsev; G. Landi; K. Lau; X. Lin; L. Lu; J. Ma; Z. Ma; G. Maccarrone; A. S. Malguin; Z. Mao; M. A. Markov; T. Massam; B. Mayes; N. Mengotti Silva; A. Misaki; G. H. Mo; B. Monteleoni; C. Morello; J. Moromisato; R. Nania; G. Navarra; L. Panaro; D. Parks; P. G. Pelfer; L. Periale; P. Picchi; P. Pinna; L. Pinsky; I. A. Pless; M. Pu; J. Pyrlyk; J. Qiu; V. G. Ryasny; O. G. Ryazhskaya; O. Saavedra; K. Saitoh; D. Sanders; G. Sartorelli; S. Sarwar; D. Shen; V. P. Talochkin; H. Tang; J. Tang; W. Tian; G. C. Trinchero; A. Turtelli; I. Uman; P. Vallania; S. Vernetto; E. von Goeler; L. Votano; T. Wada; F. Wang; H. Wang; S. Wang; R. Weathers; R. Weinstein; M. Widgoff; L. Xu; Z. Xu; V. F. Yakushev; I. Yamamoto; G. Yi; A. Zallo; G. T. Zatsepin; X. Zhou; Q. Zhu; X. Zhu; B. Zhuan; A. Zichichi

doi:10.1007/bf02740929

The most powerful scintillator supernovae detector: LVD

M. Aglietta, B. Alpat, E. D. Alyea, P. Antonioli, G. Anzivino, G. Badino, Y. Ban, G. Bari, M. Basile, A. Benelli, V. S. Berezinsky, L. Bergamasco, S. Bianco, A. Bizzetti, G. Bruni, Y. Cao, G. Cara Romeo, R. Casaccia, C. Castagnoli, A. CastellinaK. Chen, R. Chen, J. A. Chinellato, L. Cifarelli, G. Cini, S. Cong, A. Contin, V. L. Dadikin, M. Dardo, A. De Silva, M. Deutsch, L. G. Dos Santos, R. I. Enikeev, F. L. Fabbri, W. Fulgione, P. Galeotti, P. L. Ghia, P. Giusti, F. Grianti, S. Gu, E. S. Hafen, P. Haridas, G. Iacobucci, N. Inoue, F. F. Khalchukov, E. V. Korolkova, P. V. Kortchaguin, V. B. Kortchaguin, V. A. Kudryavtsev, G. Landi, K. Lau, X. Lin, L. Lu, J. Ma, Z. Ma, G. Maccarrone, A. S. Malguin, Z. Mao, M. A. Markov, T. Massam, B. Mayes, N. Mengotti Silva, A. Misaki, G. H. Mo, B. Monteleoni, C. Morello, J. Moromisato, R. Nania, G. Navarra, L. Panaro, D. Parks, P. G. Pelfer, L. Periale, P. Picchi, P. Pinna, L. Pinsky, I. A. Pless, M. Pu, J. Pyrlyk, J. Qiu, V. G. Ryasny, O. G. Ryazhskaya, O. Saavedra, K. Saitoh, D. Sanders, G. Sartorelli, S. Sarwar, D. Shen, V. P. Talochkin, H. Tang, J. Tang, W. Tian, G. C. Trinchero, A. Turtelli, I. Uman, P. Vallania, S. Vernetto, E. von Goeler, L. Votano, T. Wada, F. Wang, H. Wang, S. Wang, R. Weathers, R. Weinstein, M. Widgoff, L. Xu, Z. Xu, V. F. Yakushev, I. Yamamoto, G. Yi, A. Zallo, G. T. Zatsepin, X. Zhou, Q. Zhu, X. Zhu, B. Zhuan, A. Zichichi

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Abstract

The Large Volume Detector (LVD) in the Gran Sasso underground Laboratory is a multipurpose detector consisting of a large volume of liquid scintillator interleaved with limited streamer tubes. In this paper we discuss its power to study low-energy cosmic neutrinos. The results show that the first LVD tower (368 tons of liquid scintillator) is well suited to detect neutrinos from gravitational stellar collapses within all of our Galaxy over a wide range of burst duration (up to a few hundred seconds). No burst candidates have been observed in the first two months of data taking.

Original language	English
Pages (from-to)	1793-1804
Number of pages	12
Journal	La Rivista del Nuovo Cimento
Volume	105
Issue number	12
DOIs	https://doi.org/10.1007/bf02740929
State	Published - Dec 1992
Externally published	Yes

Keywords

94.40 - Cosmic-ray interactions with the Earth
96.40.Qr - Neutrino studies

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10.1007/bf02740929

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Aglietta, M., Alpat, B., Alyea, E. D., Antonioli, P., Anzivino, G., Badino, G., Ban, Y., Bari, G., Basile, M., Benelli, A., Berezinsky, V. S., Bergamasco, L., Bianco, S., Bizzetti, A., Bruni, G., Cao, Y., Cara Romeo, G., Casaccia, R., Castagnoli, C., ... Zichichi, A. (1992). The most powerful scintillator supernovae detector: LVD. La Rivista del Nuovo Cimento, 105(12), 1793-1804. https://doi.org/10.1007/bf02740929

@article{c43adfc532484207ad3db8b06f2c7b98,

title = "The most powerful scintillator supernovae detector: LVD",

abstract = "The Large Volume Detector (LVD) in the Gran Sasso underground Laboratory is a multipurpose detector consisting of a large volume of liquid scintillator interleaved with limited streamer tubes. In this paper we discuss its power to study low-energy cosmic neutrinos. The results show that the first LVD tower (368 tons of liquid scintillator) is well suited to detect neutrinos from gravitational stellar collapses within all of our Galaxy over a wide range of burst duration (up to a few hundred seconds). No burst candidates have been observed in the first two months of data taking.",

keywords = "94.40 - Cosmic-ray interactions with the Earth, 96.40.Qr - Neutrino studies",

author = "M. Aglietta and B. Alpat and Alyea, {E. D.} and P. Antonioli and G. Anzivino and G. Badino and Y. Ban and G. Bari and M. Basile and A. Benelli and Berezinsky, {V. S.} and L. Bergamasco and S. Bianco and A. Bizzetti and G. Bruni and Y. Cao and {Cara Romeo}, G. and R. Casaccia and C. Castagnoli and A. Castellina and K. Chen and R. Chen and Chinellato, {J. A.} and L. Cifarelli and G. Cini and S. Cong and A. Contin and Dadikin, {V. L.} and M. Dardo and {De Silva}, A. and M. Deutsch and {Dos Santos}, {L. G.} and Enikeev, {R. I.} and Fabbri, {F. L.} and W. Fulgione and P. Galeotti and Ghia, {P. L.} and P. Giusti and F. Grianti and S. Gu and Hafen, {E. S.} and P. Haridas and G. Iacobucci and N. Inoue and Khalchukov, {F. F.} and Korolkova, {E. V.} and Kortchaguin, {P. V.} and Kortchaguin, {V. B.} and Kudryavtsev, {V. A.} and G. Landi and K. Lau and X. Lin and L. Lu and J. Ma and Z. Ma and G. Maccarrone and Malguin, {A. S.} and Z. Mao and Markov, {M. A.} and T. Massam and B. Mayes and {Mengotti Silva}, N. and A. Misaki and Mo, {G. H.} and B. Monteleoni and C. Morello and J. Moromisato and R. Nania and G. Navarra and L. Panaro and D. Parks and Pelfer, {P. G.} and L. Periale and P. Picchi and P. Pinna and L. Pinsky and Pless, {I. A.} and M. Pu and J. Pyrlyk and J. Qiu and Ryasny, {V. G.} and Ryazhskaya, {O. G.} and O. Saavedra and K. Saitoh and D. Sanders and G. Sartorelli and S. Sarwar and D. Shen and Talochkin, {V. P.} and H. Tang and J. Tang and W. Tian and Trinchero, {G. C.} and A. Turtelli and I. Uman and P. Vallania and S. Vernetto and {von Goeler}, E. and L. Votano and T. Wada and F. Wang and H. Wang and S. Wang and R. Weathers and R. Weinstein and M. Widgoff and L. Xu and Z. Xu and Yakushev, {V. F.} and I. Yamamoto and G. Yi and A. Zallo and Zatsepin, {G. T.} and X. Zhou and Q. Zhu and X. Zhu and B. Zhuan and A. Zichichi",

year = "1992",

month = dec,

doi = "10.1007/bf02740929",

language = "אנגלית",

volume = "105",

pages = "1793--1804",

journal = "La Rivista del Nuovo Cimento",

issn = "0369-3546",

publisher = "Societa Italiana di Fisica",

number = "12",

}

Aglietta, M, Alpat, B, Alyea, ED, Antonioli, P, Anzivino, G, Badino, G, Ban, Y, Bari, G, Basile, M, Benelli, A, Berezinsky, VS, Bergamasco, L, Bianco, S, Bizzetti, A, Bruni, G, Cao, Y, Cara Romeo, G, Casaccia, R, Castagnoli, C, Castellina, A, Chen, K, Chen, R, Chinellato, JA, Cifarelli, L, Cini, G, Cong, S, Contin, A, Dadikin, VL, Dardo, M, De Silva, A, Deutsch, M, Dos Santos, LG, Enikeev, RI, Fabbri, FL, Fulgione, W, Galeotti, P, Ghia, PL, Giusti, P, Grianti, F, Gu, S, Hafen, ES, Haridas, P, Iacobucci, G, Inoue, N, Khalchukov, FF, Korolkova, EV, Kortchaguin, PV, Kortchaguin, VB, Kudryavtsev, VA, Landi, G, Lau, K, Lin, X, Lu, L, Ma, J, Ma, Z, Maccarrone, G, Malguin, AS, Mao, Z, Markov, MA, Massam, T, Mayes, B, Mengotti Silva, N, Misaki, A, Mo, GH, Monteleoni, B, Morello, C, Moromisato, J, Nania, R, Navarra, G, Panaro, L, Parks, D, Pelfer, PG, Periale, L, Picchi, P, Pinna, P, Pinsky, L, Pless, IA, Pu, M, Pyrlyk, J, Qiu, J, Ryasny, VG, Ryazhskaya, OG, Saavedra, O, Saitoh, K, Sanders, D, Sartorelli, G, Sarwar, S, Shen, D, Talochkin, VP, Tang, H, Tang, J, Tian, W, Trinchero, GC, Turtelli, A, Uman, I, Vallania, P, Vernetto, S, von Goeler, E, Votano, L, Wada, T, Wang, F, Wang, H, Wang, S, Weathers, R, Weinstein, R, Widgoff, M, Xu, L, Xu, Z, Yakushev, VF, Yamamoto, I, Yi, G, Zallo, A, Zatsepin, GT, Zhou, X, Zhu, Q, Zhu, X, Zhuan, B & Zichichi, A 1992, 'The most powerful scintillator supernovae detector: LVD', La Rivista del Nuovo Cimento, vol. 105, no. 12, pp. 1793-1804. https://doi.org/10.1007/bf02740929

TY - JOUR

T1 - The most powerful scintillator supernovae detector

T2 - LVD

AU - Aglietta, M.

AU - Alpat, B.

AU - Alyea, E. D.

AU - Antonioli, P.

AU - Anzivino, G.

AU - Badino, G.

AU - Ban, Y.

AU - Bari, G.

AU - Basile, M.

AU - Benelli, A.

AU - Berezinsky, V. S.

AU - Bergamasco, L.

AU - Bianco, S.

AU - Bizzetti, A.

AU - Bruni, G.

AU - Cao, Y.

AU - Cara Romeo, G.

AU - Casaccia, R.

AU - Castagnoli, C.

AU - Castellina, A.

AU - Chen, K.

AU - Chen, R.

AU - Chinellato, J. A.

AU - Cifarelli, L.

AU - Cini, G.

AU - Cong, S.

AU - Contin, A.

AU - Dadikin, V. L.

AU - Dardo, M.

AU - De Silva, A.

AU - Deutsch, M.

AU - Dos Santos, L. G.

AU - Enikeev, R. I.

AU - Fabbri, F. L.

AU - Fulgione, W.

AU - Galeotti, P.

AU - Ghia, P. L.

AU - Giusti, P.

AU - Grianti, F.

AU - Gu, S.

AU - Hafen, E. S.

AU - Haridas, P.

AU - Iacobucci, G.

AU - Inoue, N.

AU - Khalchukov, F. F.

AU - Korolkova, E. V.

AU - Kortchaguin, P. V.

AU - Kortchaguin, V. B.

AU - Kudryavtsev, V. A.

AU - Landi, G.

AU - Lau, K.

AU - Lin, X.

AU - Lu, L.

AU - Ma, J.

AU - Ma, Z.

AU - Maccarrone, G.

AU - Malguin, A. S.

AU - Mao, Z.

AU - Markov, M. A.

AU - Massam, T.

AU - Mayes, B.

AU - Mengotti Silva, N.

AU - Misaki, A.

AU - Mo, G. H.

AU - Monteleoni, B.

AU - Morello, C.

AU - Moromisato, J.

AU - Nania, R.

AU - Navarra, G.

AU - Panaro, L.

AU - Parks, D.

AU - Pelfer, P. G.

AU - Periale, L.

AU - Picchi, P.

AU - Pinna, P.

AU - Pinsky, L.

AU - Pless, I. A.

AU - Pu, M.

AU - Pyrlyk, J.

AU - Qiu, J.

AU - Ryasny, V. G.

AU - Ryazhskaya, O. G.

AU - Saavedra, O.

AU - Saitoh, K.

AU - Sanders, D.

AU - Sartorelli, G.

AU - Sarwar, S.

AU - Shen, D.

AU - Talochkin, V. P.

AU - Tang, H.

AU - Tang, J.

AU - Tian, W.

AU - Trinchero, G. C.

AU - Turtelli, A.

AU - Uman, I.

AU - Vallania, P.

AU - Vernetto, S.

AU - von Goeler, E.

AU - Votano, L.

AU - Wada, T.

AU - Wang, F.

AU - Wang, H.

AU - Wang, S.

AU - Weathers, R.

AU - Weinstein, R.

AU - Widgoff, M.

AU - Xu, L.

AU - Xu, Z.

AU - Yakushev, V. F.

AU - Yamamoto, I.

AU - Yi, G.

AU - Zallo, A.

AU - Zatsepin, G. T.

AU - Zhou, X.

AU - Zhu, Q.

AU - Zhu, X.

AU - Zhuan, B.

AU - Zichichi, A.

PY - 1992/12

Y1 - 1992/12

N2 - The Large Volume Detector (LVD) in the Gran Sasso underground Laboratory is a multipurpose detector consisting of a large volume of liquid scintillator interleaved with limited streamer tubes. In this paper we discuss its power to study low-energy cosmic neutrinos. The results show that the first LVD tower (368 tons of liquid scintillator) is well suited to detect neutrinos from gravitational stellar collapses within all of our Galaxy over a wide range of burst duration (up to a few hundred seconds). No burst candidates have been observed in the first two months of data taking.

AB - The Large Volume Detector (LVD) in the Gran Sasso underground Laboratory is a multipurpose detector consisting of a large volume of liquid scintillator interleaved with limited streamer tubes. In this paper we discuss its power to study low-energy cosmic neutrinos. The results show that the first LVD tower (368 tons of liquid scintillator) is well suited to detect neutrinos from gravitational stellar collapses within all of our Galaxy over a wide range of burst duration (up to a few hundred seconds). No burst candidates have been observed in the first two months of data taking.

KW - 94.40 - Cosmic-ray interactions with the Earth

KW - 96.40.Qr - Neutrino studies

UR - http://www.scopus.com/inward/record.url?scp=51649132596&partnerID=8YFLogxK

U2 - 10.1007/bf02740929

DO - 10.1007/bf02740929

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:51649132596

SN - 0369-3546

VL - 105

SP - 1793

EP - 1804

JO - La Rivista del Nuovo Cimento

JF - La Rivista del Nuovo Cimento

IS - 12

ER -

The most powerful scintillator supernovae detector: LVD

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Keywords

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