Il Nuovo Cimento C

, Volume 2, Issue 4, pp 473–487 | Cite as

Integral and differential absolute intensity measurements of cosmic-ray muons below 1 GeV

  • B. Baschiera
  • G. Basini
  • H. Bilokon
  • B. D'Ettorre Piazzoli
  • G. Mannocchi
  • C. Castagnoli
  • P. Picchi
Article

Summary

Absolute differential and integral muon intensities below 1 Ge V/c have been measured with a flash-tube range spectrograph in which stopping muons are identified by the decay sequence. The differential intensities at 0.314 GeV/c and 0.805 GeV/c are (3.25±0.17)·10−3 cm−2 sr−1·s−1 (GeV/c)−1 and (3.60±0.18)·10−3 cm−2 sr−1 s−1 (GeV/c)−1, respectively,i.e. 16% and 33% higher than that of Rossi. These measurements confirm the rencent results of other authors according to which the Rossi reference point at 1 GeV/c is too low of about 25%. Our integral measurements at 0.457 GeV/c and 0.918 GeV/c support this evidence.

Резюме

Измерены абсолютные дифферецниальные и интегральные интенсивности мюонов ниже 1 ГэB/c, используя спектрограф, в котором остановившиеся мюоны идентифицируются по цепочке распадов. Диффенциальные интенсивностн при 0.314 ГэB/c и 0.805 ГэB/c соответственно составляют (3.25±0.17)·10−3 см−2 ср−1 с−1 (ГэВ/с)−1 и (3.60±0.18)·10−3 см−2 ср−1 с−1 (ГэВ/с)−1, т.е. нв 16% и 33% выше результатов Росси. Проведенные измерения подтвершдают недавние результаты других авторов, согласно которым точка отсчета Росси при 1 ГэВ/с расподожена ниже на 25%. Наши интегральные измерения при 0.457 ГэВ/с и 0.918 ГэВ/с подтверждают этот результат.

Keywords

Liquid Scintillation Counter Plastic Scintillator Liquid Scintillator Muon Decay Differential Measurement 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Riassunto

Con uno spettrografo a range di tubi a flash sono state misurate le intensità differenziali e integrali sotto 1 GeV/c rivelando la catena del decadimento del muone. Le intensità differenziali a 0.314 GeV/c e 0.805 GeV/c sono rispettivamente (3.25±0.17)·10−3 cm2 sr−1 s−1 (GeV/c)−1 e (3.60±0.18)·10−3 cm−2 sr−1 s−1 (GeV/c)−1, cioè 16% e 33% più alte di quella di Rossi. Queste misure confermano i recenti risultati di altri autori secondo i quali il punto di riferimento di Rossi a 1 GeV/c è più basso di∼25%. Le nostre misure d'intensità integrale a 0.457 GeV/c e 0.918 GeV/c sostengono queste evidenze.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. (1).
    B. Rossi:Rev. Mod. Phys.,20, 537 (1948).CrossRefADSGoogle Scholar
  2. (2).
    O. C. Allkofer, W. D. Dan andH. Jokisch:Phys. Lett. B,31, 606 (1970);36, 428 (1971).CrossRefADSGoogle Scholar
  3. (3).
    F. Ashton, K. Tsuji andA. W. Wolfendale:Nuovo Cimento B,9, 344 (1972).Google Scholar
  4. (4).
    A. K. De, P. Ghosh, S. Mitra, P. C. Bhattacharya andA. K. Das:Phys. Rev. D,5, 1068 (1972).CrossRefADSGoogle Scholar
  5. (5).
    J. N. Crookes andB. C. Rastin:Nucl. Phys. B,39, 493 (1972).CrossRefADSGoogle Scholar
  6. (6).
    L. K. Ng, M. G. Thompson andM. R. Whalley:Nuovo Cimento B,22, 328 (1974).Google Scholar
  7. (7).
    D. F. L. Kong, S. Y. Lau andL. K. Ng:Proceedings of the XIV International Cosmic-Ray Conference, Vol.6 (München, 1975), p. 1852.Google Scholar
  8. (8).
    G. Mannocchi: thesis (1973), University of Rome (unpublished).Google Scholar
  9. (9).
    C. Richard-Serre: preprint CERN 71-18 (1971).Google Scholar
  10. (10).
    H. P. Koenig:Phys. Rev.,69, 590 (1946);A. Buhler, T. Massam, Th. Muller andA. Zichichi:Nuovo Cimento,35, 759 (1965).CrossRefADSGoogle Scholar
  11. (11).
    L. Eyges:Phys. Rev.,74, 1534 (1948).CrossRefADSGoogle Scholar
  12. (12).
    R. M. Sternheimer:Rev. Sci. Instrum.,25, 1070 (1954).CrossRefGoogle Scholar
  13. (13).
    O. C. Allkofer andH. Jokisch:Nuovo Cimento A,15, 371 (1973).Google Scholar
  14. (14).
    A. K. De, P. Ghosh, S. Mitra, P. C. Bhattacharya andA. K. Das:J. Phys. A,5, 1236 (1972).CrossRefADSGoogle Scholar
  15. (15).
    P. C. Bhattacharya:Z. Phys.,234, 17 (1970).CrossRefGoogle Scholar
  16. (16).
    B. J. Bateman, W. G. Coutrell, D. R. Durda, N. M. Duller, P. J. Green, A. V. Jelinek, T. A. Nagy andW. R. Sheldon:Phys. Lett. B,36, 144 (1971).CrossRefADSGoogle Scholar
  17. (17).
    K. I. Greisen:Phys. Rev.,61, 212 (1942).CrossRefADSGoogle Scholar
  18. (18).
    J. M. Paul:Nucl. Instrum. Methods,96, 51 (1971).CrossRefADSGoogle Scholar
  19. (19).
    W. Borsch-Supan:J. Res. Nat. Bur. Stand. Sect. B,65, 245 (1961).MathSciNetGoogle Scholar
  20. (20).
    E. J. Kobetich andR. Katz:Phys. Rev.,170, 391 (1968).CrossRefADSGoogle Scholar
  21. (21).
    High Energy and Nuclear Physics Data Handbook, Rutherford High Energy Laboratory (1964), Sect, VIII.Google Scholar
  22. (22).
    J. R. Prescott andP. S. Takhar:IRE Trans. Nucl. Sci., NS 9, 3, 36 (1962).Google Scholar

Copyright information

© Societá Italiana di Fisica 1979

Authors and Affiliations

  • B. Baschiera
    • 1
  • G. Basini
    • 1
    • 2
  • H. Bilokon
    • 1
    • 2
  • B. D'Ettorre Piazzoli
    • 1
    • 2
  • G. Mannocchi
    • 1
    • 2
  • C. Castagnoli
    • 3
  • P. Picchi
    • 2
    • 3
  1. 1.Laboratorio di Cosmogeofisica del CNRTorino
  2. 2.Laboratori Nazionali di FrascatiIstituto Nazionale di Fisica NucleareFrascati (Roma)
  3. 3.Istituto di Fisica Generale dell' UniversitàTorino

Personalised recommendations