Atmospheric muon flux at sea level, underground, and underwater

被引:207
作者
Bugaev, EV
Misaki, A
Naumov, VA
Sinegovskaya, TS
Sinegovsky, SI
Takahashi, N
机构
[1] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia
[2] Natl Grad Inst Policy Studies, Urawa, Saitama 3388570, Japan
[3] Irkutsk State Univ, Theoret Phys Lab, Irkutsk 664003, Russia
[4] Irkutsk State Univ, Fac Phys, Dept Theoret Phys, Irkutsk 664003, Russia
[5] Ist Nazl Fis Nucl, I-50125 Florence, Italy
[6] Hirosaki Univ, Fac Sci & Technol, Dept Elect & Informat Syst Engn, Hirosaki, Aomori 0368561, Japan
关键词
D O I
10.1103/PhysRevD.58.054001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The vertical sea-level muon spectrum at energies above 1 GeV and the muon intensities at depths up to 18 km w.e. in different rocks and in water are calculated. The results are particularly collated with a great body of the ground-level, underground, and underwater muon data. In the hadron-cascade calculations, we take into account the logarithmic growth with energy of inelastic cross sections and pion, kaon, and nucleon generation in pion-nucleus collisions. For evaluating the prompt-muon contribution to the muon flux, we apply the two phenomenological approaches to the charm production problem: the recombination quark-parton model and the quark-gluon string model. To solve the muon transport equation at large depths of a homogeneous medium, we used a semianalytical method, which allows the inclusion of an arbitrary (decreasing) muon spectrum at the medium boundary and real energy dependence of both continuous and discrete muon energy losses. The method is checked for accuracy by direct Monte Carlo calculation. Whenever possible, we give simple fitting formulas describing our numerical results. [S0556-2821(98)00313-0].
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页数:27
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共 183 条
  • [1] NUCLEAR-DEPENDENCE OF CHARM PRODUCTION BY A 340 GEV PI-BEAM
    ADAMOVICH, M
    ALEXANDROV, Y
    ANTINORI, F
    BARBERIS, D
    BEUSCH, W
    BUYS, A
    DAMERI, M
    DAVENPORT, M
    DUFEY, JP
    FORINO, A
    FRENCH, BR
    GERASIMOV, S
    GESSAROLI, R
    GRARD, F
    HURST, R
    JACHOLKOWSKI, A
    KIRK, A
    LASSALLE, JC
    LEGROS, P
    MAZZANTI, P
    MERONI, C
    MULLER, F
    OSCULATI, B
    QUARENI, A
    REDAELLI, N
    ROSSI, L
    TOMASINI, G
    TORRETTA, D
    VIAGGI, F
    ZAVERTYAEV, M
    [J]. PHYSICS LETTERS B, 1992, 284 (3-4) : 453 - 456
  • [2] Adarkav H., 1990, P 21 INT COSM RAY C, V9, P310
  • [3] Aglietta M., 1990, Nuclear Physics B, Proceedings Supplements, V14B, P193, DOI 10.1016/0920-5632(90)90380-D
  • [4] NEUTRINO-INDUCED AND ATMOSPHERIC SINGLE-MUON FLUXES MEASURED OVER 5 DECADES OF INTENSITY BY LVD AT GRAN-SASSO-LABORATORY
    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
    [J]. ASTROPARTICLE PHYSICS, 1995, 3 (04) : 311 - 320
  • [5] AGLIETTA M, 1995, UNPUB P 24 INT COSM, V1, P638
  • [6] Atmospheric neutrino flux above 1 GeV
    Agrawal, V
    Gaisser, TK
    Lipari, P
    Stanev, T
    [J]. PHYSICAL REVIEW D, 1996, 53 (03): : 1314 - 1323
  • [7] AGUILARBENITEZ M, 1988, Z PHYS C PART FIELDS, V40, P321, DOI 10.1007/BF01548848
  • [8] D-MESON PRODUCTION FROM 400 GEV/C P-P INTERACTIONS EVIDENCE FOR LEADING DI-QUARKS
    AGUILARBENITEZ, M
    ALLISON, WWM
    BAILLY, JL
    BANERJEE, S
    BARTL, W
    BEGALLI, M
    BEILLIERE, P
    BIZZARRI, R
    BRIAND, H
    CANALE, V
    CASO, C
    CASTELLI, E
    CHECCHIA, P
    CHLIAPNIKOV, PV
    COLINO, N
    COLWILL, SJ
    CONTRI, R
    CRENNELL, D
    DEANGELIS, A
    DEBILLY, L
    DEFOIX, C
    DIMARCO, R
    DICAPUA, E
    DIEZHEDO, F
    DOLBEAU, J
    DUMARCHEZ, J
    ERIKSSON, M
    FALCIANO, S
    FERNANDEZ, C
    FISHER, C
    FISYAK, YV
    FONTANELLI, F
    FREY, JR
    GANGULI, SN
    GASPARINI, U
    GENSCH, U
    GENTILE, S
    GIBAUT, DB
    GOSHAW, AT
    GRARD, F
    GURTU, A
    HAMATSU, R
    HAUPT, L
    HELLMAN, S
    HERNANDEZ, JJ
    HOLMGREN, SO
    HOULDEN, M
    HRUBEC, J
    HUGHES, P
    HUSS, D
    [J]. PHYSICS LETTERS B, 1988, 201 (01) : 176 - 182
  • [9] ALEEV AN, 1993, PHYS ATOM NUCL+, V56, P1235
  • [10] Allkofer O.C., 1984, COSMIC RAYS EARTH