LVD at Gran Sasso

C. Bari; M. Basile; G. Bruni; G. Cara Romeo; A. Castelvetri; L. Cifarelli; A. Contin; C. Del Papa; P. Giusti; G. Iacobucci; G. Maccarrone; T. Massam; R. Nania; V. O'Shea; F. Palmonari; E. Perotto; G. Prisco; G. Sartorelli; M. Willutzky; J. A. Chincellato; C. Dobrigkeit Chincellato; A. C. Fauth; A. Turtelli; K. De; A. M. Shapiro; M. Widgoff; F. Rohrbach; A. Zichichi; P. Caputi; G. L. Susino; G. Barbagli; G. Confronto; G. Landi; P. Pelfer; S. Bianco; G. Anzivino; R. Casaccia; F. Cindolo; M. Enorini; F. Fabbri; I. Laakso; S. Qian; A. Rindi; A. Spallone; L. Votano; A. Zallo; K. Lau; F. Lipps; B. Mayes; G. H. Mo; L. Pinsky; J. Pyrlik; D. Sanders; W. R. Sheldon; R. Weinstein; Y. Dai; L. Din; C. Jing; G. Jing; Z. Lu; P. Shen; Q. Zhu; D. Alyea; G. Di Sciascio; R. Scrimaglio; P. Rotelli; G. E. Kocharov; M. Deutsch; E. S. Hafen; P. Haridas; B. Jeckelmann; G. Ji; H. H. Kuang; A. Pitas; I. A. Pless; Y. Yuan; C. Z. Zhao; V. S. Berezinski; V. L. Dadykin; F. F. Khalchukov; E. V. Korolkova; P. V. Kortchaguin; V. B. Kortchaguin; V. A. Kudryavtsev; A. S. Malguin; M. A. Markov; V. G. Ryassny; O. G. Ryazhskaya; V. P. Talochkin; V. F. Yakushev; G. T. Zatsepin; J. Moromisato; E. Saletan; D. Shambroom; E. von Goeler; G. D'Ali; S. de Pasquale; B. Alpat; F. Artemi; C. Cappelletti; P. Diodati; P. Salvadori; C. Aglietta; G. Badino; L. Bergamasco; C. Castagnoli; A. Castellina; G. Cini; M. Dardo; W. Fulgione; P. Galeotti; C. Morello; G. Navarra; L. Periale; P. Picchi; O. Saavedra; G. C. Trinchero; P. Vallania; S. Vernetto; F. Grianti; F. Vetrano

doi:10.1016/0168-9002(88)91094-7

LVD at Gran Sasso

C. Bari, M. Basile, G. Bruni, G. Cara Romeo, A. Castelvetri, L. Cifarelli, A. Contin, C. Del Papa, P. Giusti, G. Iacobucci, G. Maccarrone, T. Massam, R. Nania, V. O'Shea, F. Palmonari, E. Perotto, G. Prisco, G. Sartorelli, M. Willutzky, J. A. ChincellatoC. Dobrigkeit Chincellato, A. C. Fauth, A. Turtelli, K. De, A. M. Shapiro, M. Widgoff, F. Rohrbach, A. Zichichi, P. Caputi, G. L. Susino, G. Barbagli, G. Confronto, G. Landi, P. Pelfer, S. Bianco, G. Anzivino, R. Casaccia, F. Cindolo, M. Enorini, F. Fabbri, I. Laakso, S. Qian, A. Rindi, A. Spallone, L. Votano, A. Zallo, K. Lau, F. Lipps, B. Mayes, G. H. Mo, L. Pinsky, J. Pyrlik, D. Sanders, W. R. Sheldon, R. Weinstein, Y. Dai, L. Din, C. Jing, G. Jing, Z. Lu, P. Shen, Q. Zhu, D. Alyea, G. Di Sciascio, R. Scrimaglio, P. Rotelli, G. E. Kocharov, M. Deutsch, E. S. Hafen, P. Haridas, B. Jeckelmann, G. Ji, H. H. Kuang, A. Pitas, I. A. Pless, Y. Yuan, C. Z. Zhao, V. S. Berezinski, V. L. Dadykin, F. F. Khalchukov, E. V. Korolkova, P. V. Kortchaguin, V. B. Kortchaguin, V. A. Kudryavtsev, A. S. Malguin, M. A. Markov, V. G. Ryassny, O. G. Ryazhskaya, V. P. Talochkin, V. F. Yakushev, G. T. Zatsepin, J. Moromisato, E. Saletan, D. Shambroom, E. von Goeler, G. D'Ali, S. de Pasquale, B. Alpat, F. Artemi, C. Cappelletti, P. Diodati, P. Salvadori, C. Aglietta, G. Badino, L. Bergamasco, C. Castagnoli, A. Castellina, G. Cini, M. Dardo, W. Fulgione, P. Galeotti, C. Morello, G. Navarra, L. Periale, P. Picchi, O. Saavedra, G. C. Trinchero, P. Vallania, S. Vernetto, F. Grianti, F. Vetrano

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Abstract

LVD is a large volume detector which will be installed in Hall A of the Gran Sasso Laboratory. This detector is 49 m long, 13.2 m high and 12 m wide. It contains 2280 m³ of scintillator (1800 t) and 1800 t of steel. The geometric acceptance of LVD for an isotropic flux of particles is greater than 7000 m² sr. LVD is the ideal detector for detecting a stellar collapse, anywhere in our galaxy; for studying neutrino oscillations; for searching for the supersymmetric decay mode of the proton; and for looking at the boron neutrinos from the sun. LVD is a very competitive detector for detecting astrophysical neutrino emitting point sources, for performing dark matter searches, for studying single muon distributions, for detecting muon bundles and hence determining the primary cosmic ray composition, and for searching for massive monopoles and other ultra heavy particles. LVD is composed of 190 identical modules, of which the first 10% of these modules will installed in 1987.

Original language	English
Pages (from-to)	5-17
Number of pages	13
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	264
Issue number	1
DOIs	https://doi.org/10.1016/0168-9002(88)91094-7
State	Published - 1 Feb 1988
Externally published	Yes

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10.1016/0168-9002(88)91094-7

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Bari, C., Basile, M., Bruni, G., Cara Romeo, G., Castelvetri, A., Cifarelli, L., Contin, A., Del Papa, C., Giusti, P., Iacobucci, G., Maccarrone, G., Massam, T., Nania, R., O'Shea, V., Palmonari, F., Perotto, E., Prisco, G., Sartorelli, G., Willutzky, M., ... Vetrano, F. (1988). LVD at Gran Sasso. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 264(1), 5-17. https://doi.org/10.1016/0168-9002(88)91094-7

@article{98cd81f4b9e548c993e244a02a3f0321,

title = "LVD at Gran Sasso",

abstract = "LVD is a large volume detector which will be installed in Hall A of the Gran Sasso Laboratory. This detector is 49 m long, 13.2 m high and 12 m wide. It contains 2280 m3 of scintillator (1800 t) and 1800 t of steel. The geometric acceptance of LVD for an isotropic flux of particles is greater than 7000 m2 sr. LVD is the ideal detector for detecting a stellar collapse, anywhere in our galaxy; for studying neutrino oscillations; for searching for the supersymmetric decay mode of the proton; and for looking at the boron neutrinos from the sun. LVD is a very competitive detector for detecting astrophysical neutrino emitting point sources, for performing dark matter searches, for studying single muon distributions, for detecting muon bundles and hence determining the primary cosmic ray composition, and for searching for massive monopoles and other ultra heavy particles. LVD is composed of 190 identical modules, of which the first 10% of these modules will installed in 1987.",

author = "C. Bari and M. Basile and G. Bruni and {Cara Romeo}, G. and A. Castelvetri and L. Cifarelli and A. Contin and {Del Papa}, C. and P. Giusti and G. Iacobucci and G. Maccarrone and T. Massam and R. Nania and V. O'Shea and F. Palmonari and E. Perotto and G. Prisco and G. Sartorelli and M. Willutzky and Chincellato, {J. A.} and {Dobrigkeit Chincellato}, C. and Fauth, {A. C.} and A. Turtelli and K. De and Shapiro, {A. M.} and M. Widgoff and F. Rohrbach and A. Zichichi and P. Caputi and Susino, {G. L.} and G. Barbagli and G. Confronto and G. Landi and P. Pelfer and S. Bianco and G. Anzivino and R. Casaccia and F. Cindolo and M. Enorini and F. Fabbri and I. Laakso and S. Qian and A. Rindi and A. Spallone and L. Votano and A. Zallo and K. Lau and F. Lipps and B. Mayes and Mo, {G. H.} and L. Pinsky and J. Pyrlik and D. Sanders and Sheldon, {W. R.} and R. Weinstein and Y. Dai and L. Din and C. Jing and G. Jing and Z. Lu and P. Shen and Q. Zhu and D. Alyea and {Di Sciascio}, G. and R. Scrimaglio and P. Rotelli and Kocharov, {G. E.} and M. Deutsch and Hafen, {E. S.} and P. Haridas and B. Jeckelmann and G. Ji and Kuang, {H. H.} and A. Pitas and Pless, {I. A.} and Y. Yuan and Zhao, {C. Z.} and Berezinski, {V. S.} and Dadykin, {V. L.} and Khalchukov, {F. F.} and Korolkova, {E. V.} and Kortchaguin, {P. V.} and Kortchaguin, {V. B.} and Kudryavtsev, {V. A.} and Malguin, {A. S.} and Markov, {M. A.} and Ryassny, {V. G.} and Ryazhskaya, {O. G.} and Talochkin, {V. P.} and Yakushev, {V. F.} and Zatsepin, {G. T.} and J. Moromisato and E. Saletan and D. Shambroom and {von Goeler}, E. and G. D'Ali and {de Pasquale}, S. and B. Alpat and F. Artemi and C. Cappelletti and P. Diodati and P. Salvadori and C. Aglietta and G. Badino and L. Bergamasco and C. Castagnoli and A. Castellina and G. Cini and M. Dardo and W. Fulgione and P. Galeotti and C. Morello and G. Navarra and L. Periale and P. Picchi and O. Saavedra and Trinchero, {G. C.} and P. Vallania and S. Vernetto and F. Grianti and F. Vetrano",

year = "1988",

month = feb,

day = "1",

doi = "10.1016/0168-9002(88)91094-7",

language = "אנגלית",

volume = "264",

pages = "5--17",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier B.V.",

number = "1",

}

Bari, C, Basile, M, Bruni, G, Cara Romeo, G, Castelvetri, A, Cifarelli, L, Contin, A, Del Papa, C, Giusti, P, Iacobucci, G, Maccarrone, G, Massam, T, Nania, R, O'Shea, V, Palmonari, F, Perotto, E, Prisco, G, Sartorelli, G, Willutzky, M, Chincellato, JA, Dobrigkeit Chincellato, C, Fauth, AC, Turtelli, A, De, K, Shapiro, AM, Widgoff, M, Rohrbach, F, Zichichi, A, Caputi, P, Susino, GL, Barbagli, G, Confronto, G, Landi, G, Pelfer, P, Bianco, S, Anzivino, G, Casaccia, R, Cindolo, F, Enorini, M, Fabbri, F, Laakso, I, Qian, S, Rindi, A, Spallone, A, Votano, L, Zallo, A, Lau, K, Lipps, F, Mayes, B, Mo, GH, Pinsky, L, Pyrlik, J, Sanders, D, Sheldon, WR, Weinstein, R, Dai, Y, Din, L, Jing, C, Jing, G, Lu, Z, Shen, P, Zhu, Q, Alyea, D, Di Sciascio, G, Scrimaglio, R, Rotelli, P, Kocharov, GE, Deutsch, M, Hafen, ES, Haridas, P, Jeckelmann, B, Ji, G, Kuang, HH, Pitas, A, Pless, IA, Yuan, Y, Zhao, CZ, Berezinski, VS, Dadykin, VL, Khalchukov, FF, Korolkova, EV, Kortchaguin, PV, Kortchaguin, VB, Kudryavtsev, VA, Malguin, AS, Markov, MA, Ryassny, VG, Ryazhskaya, OG, Talochkin, VP, Yakushev, VF, Zatsepin, GT, Moromisato, J, Saletan, E, Shambroom, D, von Goeler, E, D'Ali, G, de Pasquale, S, Alpat, B, Artemi, F, Cappelletti, C, Diodati, P, Salvadori, P, Aglietta, C, Badino, G, Bergamasco, L, Castagnoli, C, Castellina, A, Cini, G, Dardo, M, Fulgione, W, Galeotti, P, Morello, C, Navarra, G, Periale, L, Picchi, P, Saavedra, O, Trinchero, GC, Vallania, P, Vernetto, S, Grianti, F & Vetrano, F 1988, 'LVD at Gran Sasso', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 264, no. 1, pp. 5-17. https://doi.org/10.1016/0168-9002(88)91094-7

TY - JOUR

T1 - LVD at Gran Sasso

AU - Bari, C.

AU - Basile, M.

AU - Bruni, G.

AU - Cara Romeo, G.

AU - Castelvetri, A.

AU - Cifarelli, L.

AU - Contin, A.

AU - Del Papa, C.

AU - Giusti, P.

AU - Iacobucci, G.

AU - Maccarrone, G.

AU - Massam, T.

AU - Nania, R.

AU - O'Shea, V.

AU - Palmonari, F.

AU - Perotto, E.

AU - Prisco, G.

AU - Sartorelli, G.

AU - Willutzky, M.

AU - Chincellato, J. A.

AU - Dobrigkeit Chincellato, C.

AU - Fauth, A. C.

AU - Turtelli, A.

AU - De, K.

AU - Shapiro, A. M.

AU - Widgoff, M.

AU - Rohrbach, F.

AU - Zichichi, A.

AU - Caputi, P.

AU - Susino, G. L.

AU - Barbagli, G.

AU - Confronto, G.

AU - Landi, G.

AU - Pelfer, P.

AU - Bianco, S.

AU - Anzivino, G.

AU - Casaccia, R.

AU - Cindolo, F.

AU - Enorini, M.

AU - Fabbri, F.

AU - Laakso, I.

AU - Qian, S.

AU - Rindi, A.

AU - Spallone, A.

AU - Votano, L.

AU - Zallo, A.

AU - Lau, K.

AU - Lipps, F.

AU - Mayes, B.

AU - Mo, G. H.

AU - Pinsky, L.

AU - Pyrlik, J.

AU - Sanders, D.

AU - Sheldon, W. R.

AU - Weinstein, R.

AU - Dai, Y.

AU - Din, L.

AU - Jing, C.

AU - Jing, G.

AU - Lu, Z.

AU - Shen, P.

AU - Zhu, Q.

AU - Alyea, D.

AU - Di Sciascio, G.

AU - Scrimaglio, R.

AU - Rotelli, P.

AU - Kocharov, G. E.

AU - Deutsch, M.

AU - Hafen, E. S.

AU - Haridas, P.

AU - Jeckelmann, B.

AU - Ji, G.

AU - Kuang, H. H.

AU - Pitas, A.

AU - Pless, I. A.

AU - Yuan, Y.

AU - Zhao, C. Z.

AU - Berezinski, V. S.

AU - Dadykin, V. L.

AU - Khalchukov, F. F.

AU - Korolkova, E. V.

AU - Kortchaguin, P. V.

AU - Kortchaguin, V. B.

AU - Kudryavtsev, V. A.

AU - Malguin, A. S.

AU - Markov, M. A.

AU - Ryassny, V. G.

AU - Ryazhskaya, O. G.

AU - Talochkin, V. P.

AU - Yakushev, V. F.

AU - Zatsepin, G. T.

AU - Moromisato, J.

AU - Saletan, E.

AU - Shambroom, D.

AU - von Goeler, E.

AU - D'Ali, G.

AU - de Pasquale, S.

AU - Alpat, B.

AU - Artemi, F.

AU - Cappelletti, C.

AU - Diodati, P.

AU - Salvadori, P.

AU - Aglietta, C.

AU - Badino, G.

AU - Bergamasco, L.

AU - Castagnoli, C.

AU - Castellina, A.

AU - Cini, G.

AU - Dardo, M.

AU - Fulgione, W.

AU - Galeotti, P.

AU - Morello, C.

AU - Navarra, G.

AU - Periale, L.

AU - Picchi, P.

AU - Saavedra, O.

AU - Trinchero, G. C.

AU - Vallania, P.

AU - Vernetto, S.

AU - Grianti, F.

AU - Vetrano, F.

PY - 1988/2/1

Y1 - 1988/2/1

N2 - LVD is a large volume detector which will be installed in Hall A of the Gran Sasso Laboratory. This detector is 49 m long, 13.2 m high and 12 m wide. It contains 2280 m3 of scintillator (1800 t) and 1800 t of steel. The geometric acceptance of LVD for an isotropic flux of particles is greater than 7000 m2 sr. LVD is the ideal detector for detecting a stellar collapse, anywhere in our galaxy; for studying neutrino oscillations; for searching for the supersymmetric decay mode of the proton; and for looking at the boron neutrinos from the sun. LVD is a very competitive detector for detecting astrophysical neutrino emitting point sources, for performing dark matter searches, for studying single muon distributions, for detecting muon bundles and hence determining the primary cosmic ray composition, and for searching for massive monopoles and other ultra heavy particles. LVD is composed of 190 identical modules, of which the first 10% of these modules will installed in 1987.

AB - LVD is a large volume detector which will be installed in Hall A of the Gran Sasso Laboratory. This detector is 49 m long, 13.2 m high and 12 m wide. It contains 2280 m3 of scintillator (1800 t) and 1800 t of steel. The geometric acceptance of LVD for an isotropic flux of particles is greater than 7000 m2 sr. LVD is the ideal detector for detecting a stellar collapse, anywhere in our galaxy; for studying neutrino oscillations; for searching for the supersymmetric decay mode of the proton; and for looking at the boron neutrinos from the sun. LVD is a very competitive detector for detecting astrophysical neutrino emitting point sources, for performing dark matter searches, for studying single muon distributions, for detecting muon bundles and hence determining the primary cosmic ray composition, and for searching for massive monopoles and other ultra heavy particles. LVD is composed of 190 identical modules, of which the first 10% of these modules will installed in 1987.

UR - http://www.scopus.com/inward/record.url?scp=0023291155&partnerID=8YFLogxK

U2 - 10.1016/0168-9002(88)91094-7

DO - 10.1016/0168-9002(88)91094-7

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AN - SCOPUS:0023291155

SN - 0168-9002

VL - 264

SP - 5

EP - 17

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

IS - 1

ER -

LVD at Gran Sasso

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