Il Nuovo Cimento (1955-1965)

, Volume 22, Issue 2, pp 235–250 | Cite as

Investigation of azimuthai effects at multiple particle production

  • S. A. Azimov
  • L. P. Chernova
  • G. M. Chernov
  • V. M. Chudakov
  • B. K. Nikishin


The azimuthal angular distribution of the secondary particles produced at p-N collisions of 9 GeV energy and nuclear interactions of single charged cosmic ray particles in the photoemulsion have been investigated by the suggested method. The influence of the energymomentum conservation law was estimated. The experimental results were compared with some theories and models of nuclear interactions produced by high energy nucleons.


Abbiamo studiato col metodo proposto la distribuzione azimutale angolare delle particelle secondarie prodotte in collisioni p-N di 9 GeV e in interazioni nucleari di singole particelle cariche dei raggi cosmici nelle emulsioni fotograflohe. Abbiamo valutato l’influenza della legge di conservazione dell’energia-impulso. I risultati sperimentali sono stati confrontati con alcune teorie e modelli per le interazioni nucleari prodotte da nucleoni di alta energia.


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  1. (1).
    W. L. Kraushaar andL. J. Marks:Phys. Rev.,93, 326 (1954).ADSCrossRefGoogle Scholar
  2. (2).
    Z. Koba and8. Takagi:Nuovo Cimento,10, 755 (1958).CrossRefGoogle Scholar
  3. (3).
    J. Pernegr, V. Petržilka andV. Šimak:Transactions of the International Conference on Cosmic Rays, vol.1 (Moscow, 1960), p. 119.Google Scholar
  4. (4).
    A. P. Zhdanov, I. M. Kuks, N. V. Skirda andR. M. Jakovlev:Transactions of the International Conference on Cosmic Rays, vol.1 (Moscow, 1960), p. 87.Google Scholar
  5. (5).
    D. P. Stern:Suppl. Nuovo Cimento,16, 251 (1960).CrossRefGoogle Scholar
  6. (6).
    E. M. Friedlöandek:Žurn. Èksp. Theor. Vie.,39, 965 (1960).Google Scholar
  7. (7).
    I. I. Gurevich, A. P. Mishakova, B. A. Nikol’skij andL. V. Surkova:Žurn. Éksp. Theor. Fie.,34, 265 (1958).Google Scholar
  8. (8).
    Phen Su, G. B. Zhdanov andI. Tretjakova Transactions of the International Conference on Cosmic Rays, vol.1, (Moscow, 1960) p. 111.Google Scholar
  9. (9).
    V. Smirnov andV. Dunin-Barkovskij Short Course of Mathematical Statistics for Technical Applications (Moscow, 1959).Google Scholar
  10. (10).
    S.N. Bernstein:Theory of Probabilities (Moskow-Leningrad, 1934).Google Scholar
  11. (11).
    Wang Shu-Fen, T. Vishki, I. M. Gramenitskii, U. G. Grishin, N. Dalkhazhav, R. M. Lebedev, A. A. Nomofilov, M. I. Podgoretskii andV. N. Stel’tson:Žurn. Èksp. Theor. Fiz.,39, 957 (1960).Google Scholar
  12. (12).
    E. R. T. Awunor-Renner, L. Blaskovitch, B. R. Trench, C. Ghesquière, I. B. de Minvielle-Devaux, W. W. Neale, C. Pelletier, P. Rivet, A. B. Sahiab andI. O. Skillicorn:Nuovo Cimento,17, 134 (1960).CrossRefGoogle Scholar
  13. (13).
    G. I. Kopylov: preprint JINR, P-259 (1959).Google Scholar
  14. (14).
    H. W. Meier:Nuovo Cimento,11, 307 (1959).CrossRefGoogle Scholar
  15. (15).
    Ju. A. Romanov andD. S. Cernavskij:Žurn. Èksp. Theor. Fiz.,38, 1132 (1960);D. S. Cernavskij:Suppl. Nuovo Cimento,8, 775 (1958).Google Scholar
  16. (16).
    I. M. Dremin andD. S. Cernavskij:Žurn. Èksp. Theor. Fie.,38, 228 (1960).Google Scholar
  17. (17).
    J. Gierula, M. Miesowicz andP. Zielinski:Nuovo Cimento,18, 102 (1960).CrossRefGoogle Scholar
  18. (18).
    J. Pernegr, V. Šimak andM. Votruba:Nuovo Cimento,17, 129 (1960).CrossRefGoogle Scholar
  19. (l9).
    P. Ciok, T. Coghen, J. Gierula, R. Holyński, A. Jurak, M. Miesowicz, andT. Saniewska:Nuovo Cimento,10, 741 (1958).CrossRefGoogle Scholar
  20. (20).
    B. A. Nicol’skij andA. P. Mishakova:Žurn. Èksp. Theor. Fiz.,38, 1507 (1960).Google Scholar

Copyright information

© Società Italiana di Fisica 1961

Authors and Affiliations

  • S. A. Azimov
    • 1
  • L. P. Chernova
    • 1
  • G. M. Chernov
    • 1
  • V. M. Chudakov
    • 1
  • B. K. Nikishin
    • 1
  1. 1.Physical-Technical Institute of the Academy of Sciences of the Uzbek SSRTashkent

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