Skip to main content
Log in

Experimental results on the proton-nucleus collisions at 27 GeV in emulsion

  • Published:
Il Nuovo Cimento (1955-1965)

Summary

We are examining the caracteristics of 3 226 stars produced by collisions of 27 GeV protons against emulsions nuclei. We obtain the mean multiplicities ns = 6.6 + 0.1,n h= 7.2±0.2. The mean energy of the secondary shower particles is 2.3 ±0.2 GeV. The energy transfer to the secondary mesons in the l.s. isK ∼ 0.6. From the study of the angular distribution we obtain the mean number of collisions inside the nucleus to be 1.1 and 27 for light anf heavy nuclei respectively. The mean free path for absorption is λ =38.0±1.0 which according to an optical model corresponds to a. nuclear mean free path λn = (4.3±0.3) fermi.

Riassunto

Abbiamo esaminato le caratteristiche di 3226 stelle prodotte da protoni di 27 GeV contro nuclei delle emulsioni. Per le molteplicità medie si è ottenuto ns = 6.6±0.1;n h= 7.2±0.2. L’energia media dei secondari è stata valutata con un metodo indiretto ed è risultata di 2.3±0.2 GeV. La frazione di energia trasferita ai mesoni secondari nel s.l. ć K∼ 0.6. Dallo studio della distribuzione angolare abbiamo ricavato che il numero medio di collisioni all’interno del nucleo è di 1.1 e 2.7 rispettivamente per i nuclei leggeri e pesanti. 1l cammino libero medio di assorbimento è λ=38.0±1.0 da cui con un modello ottico, si ottiene un λn in materia nucleare uguale a 4.3±0.3 fermi.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. B. Dayton, W. Koch, M. Nikolić, H. Winzeler, J. C. Combe, W. M. Gibson, W. O. Lock, M. Schneeberger andG. Vanderhaeghe:Helv. Phys. Acta,33, 544 (1960).

    Google Scholar 

  2. G. Cocconi, A. N. Diddens, E. Lillethun andA. M. Wetherell:Phys. Rev. Lett.,6, 231 (1961).

    Article  ADS  Google Scholar 

  3. A. Winzeler, B. Klaiber, W. Koch, N. Nikolić andM. Scheeberger:Nuovo Cimento,17, 8 (1960);

    Article  Google Scholar 

  4. N. P. Bogachev, S. A. Bunjatov, T. P. Merckov andV. M. Sidokov:Dokl. Akad. Nauk USSR,121, 617 (1958);

    Google Scholar 

  5. G. Cvijanovich, B. Dayton, P. Egli, B. Klaiber, W. Koch, M. Nicolić, R. Schneebergee, H. Winzelee, J. C. Combe, W. M. Gibson, W. O. Lock, M. Schneeberger andG. Vanderhaege:Nuovo Cimento,20, 1012 (1961).

    Article  Google Scholar 

  6. M. W. Teuchee andE. Loehmann: (unpublished: reported by Cirjanovich).

  7. W. R. Johnson:Phys. Rev:,99, 1049 (1955);

    Article  ADS  Google Scholar 

  8. M. Schein, D. M. Haskin andR. G. Glasser:Nuovo Cimento,3, 131 (1956).

    Article  Google Scholar 

  9. (3) (a)

  10. P. L. Jain andH. C. Glahe:Phys. Rev.,116, 458 (1959).

    Article  ADS  Google Scholar 

  11. I. M. Gramenitskii, M. Ia. Danysii, V. B. Liubimov, M. I. Podgoeetskii andD. Tuvdendorzh:Soviet Phys. JEPT,8 (35), 381 (1959);V. S. Barashenkov, V. A. Beliakov, V. V. Glagolev, N. Dalkhazhan, Yao Tsyng Se, L. F. Kirillova, E. M. Lebedev, V. M. Maltsev, P. K. Markov, N. G. Shafranova, K. D. Tolstov, E. N. Tsiganov andWang Siiou Feng:Nucl. Phys.,14, 522 (196C).

    Google Scholar 

  12. C. Beicman, M. Csejthey-Barth, J. P. Lagnaux andJ. Sacton:Nuovo Cimento,20, 1017 (1861).

    Article  Google Scholar 

  13. present work.

  14. C. W. Smith, C. P. Leavitt, A. M. Shapieo, C. E. Swartz andM. Widgoff:Phys. Rev.,92, 851 (1953).

    Google Scholar 

  15. (4)a).

  16. (4)b).

  17. (3)a.

  18. G. L. Bayatjan, I. M. Gramenitskii, A. A. Nomopilov, N. I. Podgoeetskii andE. S. Skezypezak:Soviet Phys. JEPT,9(36), 483 (1959).

    Google Scholar 

  19. (4)e).

  20. (4)f).

  21. (3)c).

  22. present work.

  23. G. B. Zhdanov, P. K. Markov, V. N. Strelstsov, M. I. Tretyakova, Oheng-Pu-Ying andM. G. Shafranova:Soviet Phys. JEPT,10(37), 433 (1960).

    Google Scholar 

  24. E. M. FriedlÄnder:Nuovo Cimento,14, 796 (1959).

    Article  Google Scholar 

  25. S. Z. Belen’kji andG. A. Milekhin:Soviet Phys. JEPT,2 (29), 14 (1956);S. Z. Belen’kji andL. D. Landau:Suppl. Nuovo Cimento,3, 15, (1956).

    Google Scholar 

  26. M. Blau andA. R. Oliver:Phys. Rev.,102, 489 (1956);

    Article  ADS  Google Scholar 

  27. Rome group: unpublished results.

  28. Shutt-Kalbach: in press.

  29. C. Besson, J. Crussard, V. Fouché, J. Hennessy, G. Kayas, V. R. Parikii andG. Trilling:Nuovo Cimento,6, 1168 (1959)

    Article  Google Scholar 

  30. H. H. Aly, J. G. M. Duthie andC. M. Fisher:Phil. Mag.,4, 993 (1959).

    Article  ADS  Google Scholar 

  31. E. M. FriedlÄnder, M. Marcu andM. Spirchez:Nuovo Cimento,18, 623 (1960)

    Article  Google Scholar 

  32. Rome group: in press.

  33. R. Hagedorn:Nuovo Cimento,15, 434 (1960).

    Article  Google Scholar 

  34. N. P. Bogachev, S.A. Bunatov, T. Vishki, Yu P. Merekov. V. M. Sidorov andV. A. Yarra:Soviel Phys. JEPT. 11 (38), 317 (1960).

    Google Scholar 

  35. W. S. Barashenkov el al.: (4)e).

  36. C. Castagnoli, G. Cortini, A. Manpredini andD. Moreno:Nuovo Cimento,10, 1539 (1960).

    Article  Google Scholar 

  37. T. Gozani andK. Sitte:Nuovo Cimento,11, 26 (1959).

    Article  Google Scholar 

  38. V. S. Barashenkov:Sov. Phys. Usp.,3, 689 (1961).

    Article  ADS  Google Scholar 

  39. Liège, Paris, Paema, Rome groups: in press.

Download references

Author information

Authors and Affiliations

Authors

Additional information

On leave from Istituto di Fisica, Università di Torino.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Barbaro-Galtieki, A., Manfredini, A., Quassiati, B. et al. Experimental results on the proton-nucleus collisions at 27 GeV in emulsion. Nuovo Cim 21, 469–483 (1961). https://doi.org/10.1007/BF02771800

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02771800

Navigation