The high energy muon spectrum in Extensive Air Showers: first data from LVD and EAS-TOP at Gran Sasso

被引：7

作者：

Aglietta, M ^{[1
]}

Alessandro, B

Alpat, B

Alyea, ED

Antonioli, P

Arneodo, F

Badino, G

Bari, G

Basile, M

Berezinsky, VS

Bergamasco, L

Bersani, F

Bertaina, M

Bertoni, R

Bonoli, G

Bosco, A

Bruni, G

Fauth, AC

Romeo, GC

Castagnoli, C

Castellina, A

Chiavassa, A

Chinellato, JA

Cifarelli, L

Cindolo, F

Castagnoli, GC

Conforto, G

Contin, A

Dadykin, VL

De Silva, A

Deutsch, M

Piazzoli, BD

Di Sciascio, G

Dominici, P

Dos Santos, LG

Emaldi, L

Enikeev, RI

Fabbri, FL

Fulgione, W

Galeotti, P

Ghetti, C

Ghia, PL

Giusti, P

Granella, R

Grianti, F

Guidi, G

Hafen, ES

Haridas, P

Iacobucci, G

Iacovacci, M

机构：

[1] Univ Bologna, Bologna, Italy

[2] Ist Nazl Fis Nucl, I-40126 Bologna, Italy

[3] Brown Univ, Providence, RI 02912 USA

[4] Univ Campinas, Campinas, Brazil

[5] Ist Nazl Fis Nucl, LNF, Frascati, Italy

[6] Ist Nazl Fis Nucl, LNGS, Assergi, Italy

[7] Univ Houston, Houston, TX USA

[8] Indiana Univ, Bloomington, IN USA

[9] MIT, Cambridge, MA 02139 USA

[10] Northeastern Univ, Boston, MA 02115 USA

[11] Russian Acad Sci, Inst Nucl Res, Moscow, Russia

[12] Okayama Univ, Okayama 700, Japan

[13] Okayama Univ Sci, Okayama 700, Japan

[14] Univ Perugia, I-06100 Perugia, Italy

[15] Ist Nazl Fis Nucl, I-06100 Perugia, Italy

[16] Saitama Univ, Urawa, Saitama, Japan

[17] Ashikaga Inst Technol, Ashikaga, Japan

[18] Univ Turin, CNR, Inst Cosmo Geophys, Turin, Italy

[19] Ist Nazl Fis Nucl, I-10125 Turin, Italy

[20] Univ Urbino, Florence, Italy

[21] Ist Nazl Fis Nucl, I-50125 Florence, Italy

[22] Univ Aquila, I-67100 Laquila, Italy

[23] Univ Naples, Naples, Italy

[24] Ist Nazl Fis Nucl, I-80125 Naples, Italy

来源：

ASTROPARTICLE PHYSICS | 1998年 / 9卷 / 03期

关键词：

D O I：

10.1016/S0927-6505(98)00024-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present evidence for a dependence of the average deep underground muon energies on shower size in the coincident EAS-TOP and LVD data at the Gran Sasso laboratories. The measured relation agrees with a mixed chemical composition of the cosmic ray primary spectrum at energies around 10(15) eV. (C) 1998 Elsevier Science B.V.

引用

页码：185 / 192

页数：8

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