CAN WE UNDERSTAND HIGH-ENERGY COSMIC-RAY SPECTRA ON BASIS OF SCALING HYPOTHESIS

被引：11

作者：

KASAHARA, K

TAKAHASHI, Y

机构：

[1] UNIV TOKYO,INST NUCL STUDY,TOKYO,JAPAN

[2] OSAKA UNIV,FAC ENGN SCI,OSAKA,JAPAN

来源：

PROGRESS OF THEORETICAL PHYSICS | 1976年 / 55卷 / 06期

关键词：

D O I：

10.1143/PTP.55.1896

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

页码：1896 / 1911

页数：16

共 43 条

[1]

AKASHI M, 1975, 14 P INT C COSM RAYS, V6, P2037

[2]

AKASHI M, 1975, 14TH INT COSM RAY C, V3, P2555

[3]

AKASHI M, 1975, 14 P INT COSM RAY C, V7, P2549

[4]

ANTONOV RA, 1971, P INT C COSMIC RAYS, V6, P2194

[5]

AUBERT JJ, 1974, PHYS REV LETT, V33, P1403

[6]

AUGUSTIN JE, 1974, PHYS REV LETT, V33, P1401

[7] PRELIMINARY RESULT OF FRASCATI (ADONE) ON NATURE OF A NEW 3.1-GEV PARTICLE PRODUCED IN E+E- ANNIHILATION [J].

BACCI, C ;

CELIO, RB ;

BERNAROD.M ;

CATON, G ;

DELFABBR.R ;

GRILLI, M ;

IAROCCI, E ;

LOCCI, M ;

MENCUCCINI, C ;

MURTAS, GP ;

PENSO, G ;

SPINETTI, GS ;

SPANO, M ;

STELLA, B ;

VALENTE, V ;

BARTOLI, B ;

BISELLO, D ;

ESPOSITO, B ;

FELICETTI, F ;

MONACELLI, P ;

NIGRO, M ;

PAOLUFI, L ;

PERUZZI, I ;

MORTEMI, GP ;

PICCOLO, M ;

RONGA, F ;

SEBASTIANI, F ;

TRASATTI, L ;

VANOLI, F ;

BARBARINO, G ;

BARBIELLINI, G ;

BEMPORAD, C ;

BIANCASTELLI, R ;

CEVENINI, F ;

CELVETTI, M ;

COSTANTINI, F ;

LARICCIA, P ;

PARASCANDALO, P ;

SASSI, E ;

SPENCER, C ;

TORTORA, L ;

TROYA, U ;

VITALE, S .

PHYSICAL REVIEW LETTERS, 1974, 33 (23) :1408-1410

[8]

BAKER WF, 1974, 17TH P INT C HIGH EN

[9] SCALING BEHAVIOR IN PP-!PI+ ANYTHING AT HIGH ENERGY [J].

BALI, NF ;

BROWN, LS ;

PECCEI, RD ;

PIGNOTTI, A .

PHYSICAL REVIEW LETTERS, 1970, 25 (08) :557-&

[10]

BELL CJ, 1973, 13 P INT C COSM RAYS, V4, P2519

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