Study of single muons with the large volume detector at the Gran Sasso Laboratory

被引:15
作者
Aglietta, M [1 ]
Alyea, ED
Antonioli, P
Badino, G
Bari, G
Basile, M
Berezinsky, VS
Bersani, F
Bertaina, M
Bertoni, R
Bruni, G
Romeo, GC
Castagnoli, C
Castellina, A
Chiavassa, A
Chinellato, JA
Cifarelli, L
Cindolo, F
Contin, A
Dadykin, VL
Dos Santos, LG
Enikeev, RI
Fulgione, W
Galeotti, P
Ghia, P
Giusti, P
Gomez, F
Granella, R
Grianti, F
Gurentsov, VI
Iacobucci, G
Inoue, N
Kemp, E
Khalchukov, FF
Korolkova, EV
Korchaguin, PV
Korchaguin, VB
Kudryavtsev, VA
Luvisetto, M
Malguin, AS
Massam, T
Silva, NM
Morello, C
Nania, R
Navarra, G
Periale, L
Pesci, A
Picchi, P
Pless, IA
Ryazhskaya, OG
机构
[1] Univ Turin, Turin, Italy
[2] CNR, Inst Cosmogeophys, I-00185 Rome, Italy
[3] Ist Nazl Fis Nucl, Turin, Italy
[4] Indiana Univ, Bloomington, IN USA
[5] Univ Bologna, Bologna, Italy
[6] Ist Nazl Fis Nucl, I-40126 Bologna, Italy
[7] Russian Acad Sci, Inst Nucl Res, Moscow, Russia
[8] MIT, Cambridge, MA 02139 USA
[9] Univ Campinas, Campinas, SP, Brazil
[10] Saitama Univ Sci, Urawa, Saitama, Japan
[11] Ist Nazl Fis Nucl, LNGS, Assergi, Italy
[12] Okayama Univ, Okayama, Japan
[13] Ist Nazl Fis Nucl, LNGS, Frascati, Italy
[14] Univ Houston, Houston, TX USA
[15] Brown Univ, Providence, RI 02912 USA
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1134/1.1540666
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The present study is based on the sample of 2.9 x 10(6) single muons observed by the Large Volume Detector (LVD) at the underground Gran Sasso Laboratory during 36 500 live hours from June 1992 to February 1998. We have measured the muon intensity at slant depths from 3 to 20 km w.e.. Most events are high-energy downward muons produced by meson decay in the atmosphere. The analysis of these muons has revealed the power index gamma of the 7 and K spectrum: gamma = 2.76 +/- 0.05. The remainders are horizontal muons produced by the neutrino interactions in the rock surrounding the LVD. The value of this flux near 90degrees is (6.1 +/- 2.7) x 10(-13) cm(-2) s(-1) sr(-1). The results are compared with the Monte Carlo simulations and the world data. (C) 2003 MAIK "Nauka/Interperiodica".
引用
收藏
页码:123 / 129
页数:7
相关论文
共 31 条
[1]   Muon "depth-intensity" relation measured by the LVD underground experiment and cosmic-ray muon spectrum at sea level [J].
Aglietta, M ;
Alpat, B ;
Alyea, ED ;
Antonioli, P ;
Badino, G ;
Bari, G ;
Basile, M ;
Berezinsky, VS ;
Bersani, F ;
Bertaina, M ;
Bertoni, R ;
Bonoli, G ;
Bosco, A ;
Bruni, G ;
Romeo, GC ;
Castagnoli, C ;
Castellina, A ;
Chiavassa, A ;
Chinellato, JA ;
Cifarelli, L ;
Cindolo, F ;
Conforto, G ;
Contin, A ;
Dadykin, VL ;
De Silva, A ;
Deutsch, M ;
Dominici, P ;
Dos Santos, LG ;
Emaldi, L ;
Enikeev, RI ;
Fabbri, FL ;
Fulgione, W ;
Galeotti, P ;
Ghetti, C ;
Ghia, P ;
Giusti, P ;
Granella, R ;
Grianti, F ;
Guidi, G ;
Hafen, ES ;
Haridas, P ;
Iacobucci, G ;
Inoue, N ;
Kemp, E ;
Khalchukov, FF ;
Korolkova, EV ;
Korchaguin, PV ;
Korchaguin, VB ;
Kudryavtsev, VA ;
Lau, K .
PHYSICAL REVIEW D, 1998, 58 (09)
[2]   Upper limit on the prompt muon flux derived from the LVD underground experiment -: art. no. 112001 [J].
Aglietta, M ;
Alpat, B ;
Alyea, ED ;
Antonioli, P ;
Badino, G ;
Bari, G ;
Basile, M ;
Berezinsky, VS ;
Bersani, F ;
Bertaina, M ;
Bertoni, R ;
Bonoli, G ;
Bosco, A ;
Bruni, G ;
Romeo, GC ;
Castagnoli, C ;
Castellina, A ;
Chiavassa, A ;
Chinellato, JA ;
Cifarelli, L ;
Cindolo, F ;
Conforto, G ;
Contin, A ;
Dadykin, VL ;
De Silva, A ;
Deutsch, M ;
Dominici, P ;
Dos Santos, LG ;
Emaldi, L ;
Enikeev, RI ;
Fabbri, FL ;
Fulgione, W ;
Galeotti, P ;
Ghetti, C ;
Ghia, P ;
Giusti, P ;
Granella, R ;
Grianti, F ;
Güidi, G ;
Hafen, ES ;
Haridas, P ;
Iacobucci, G ;
Inoue, N ;
Kemp, E ;
Khalchukov, FF ;
Korolkova, EV ;
Korchaguin, PV ;
Korchaguin, VB ;
Kudryavtsev, VA ;
Lau, K .
PHYSICAL REVIEW D, 1999, 60 (11)
[3]   NEUTRINO-INDUCED AND ATMOSPHERIC SINGLE-MUON FLUXES MEASURED OVER 5 DECADES OF INTENSITY BY LVD AT GRAN-SASSO-LABORATORY [J].
AGLIETTA, M ;
ALPAT, B ;
ALYEA, ED ;
ANTONIOLI, P ;
BADINO, G ;
BAN, Y ;
BARI, G ;
BASILE, M ;
BENELLI, A ;
BEREZINSKY, VS ;
BERTONI, R ;
BIANCO, S ;
BIZZETI, A ;
BOSCO, A ;
BRUGNOLA, G ;
BRUNI, G ;
CAO, Y ;
ROMEO, GC ;
CASTAGNOLI, C ;
CASTELLINA, A ;
CHEN, K ;
CHEN, R ;
CHIAVASSA, A ;
CHINELLATO, JA ;
CIFARELLI, L ;
CINDOLO, F ;
CONFORTO, G ;
CONG, S ;
CONTIN, A ;
DADYKIN, VL ;
DESIATI, P ;
DEPASQUALE, S ;
DESILVA, A ;
DEUTSCH, M ;
DOMINICI, P ;
DOSSANTOS, LG ;
ENIKEEV, RI ;
FABBRI, FL ;
FULGIONE, W ;
GALEOTTI, P ;
GHIA, P ;
GIUSTI, P ;
GRIANTI, F ;
GU, S ;
GUIDI, G ;
GUO, Y ;
HAFEN, ES ;
HARIDAS, P ;
IACOBUCCI, G ;
INOUE, N .
ASTROPARTICLE PHYSICS, 1995, 3 (04) :311-320
[4]  
AGLIETTA M, 1999, P 26 INT COSM RAY C, V7, P218
[5]   Atmospheric neutrino flux above 1 GeV [J].
Agrawal, V ;
Gaisser, TK ;
Lipari, P ;
Stanev, T .
PHYSICAL REVIEW D, 1996, 53 (03) :1314-1323
[6]  
ALLKOFER OC, 1981, 17TH P INT C COSM RA, V10, P321
[7]   Probing Higgs sector CP violation with top quarks at a photon linear collider [J].
Anlauf, H ;
Bernreuther, W ;
Brandenburg, A .
PHYSICAL REVIEW D, 1995, 52 (07) :3803-3808
[8]  
Andreev Yu.M., 1987, P 20 INT COSM RAY C, V6, P200
[9]   A three-dimensional code for muon propagation through the rock: MUSIC [J].
Antonioli, P ;
Ghetti, C ;
Korolkova, EV ;
Kudryavtsev, VA ;
Sartorelli, G .
ASTROPARTICLE PHYSICS, 1997, 7 (04) :357-368
[10]  
ASHITKOV VD, 1985, P 19 INT COSM RAY C, V8, P77