- Autor(in)
- Referenz
-
1 Boehmer, H. W., and H. S. Bridge, Phys. Rev., 85 (1952) 863.
2 Walker, W. D., and S. P. Walker and K. I. Greisen, Phys. Rev., 80 (1951) 546.
3 Gregory, B. P., and J. H. Tinlot, Phys. Rev., 81 (1951) 675.
4 Barrett, P. H., Phys. Rev., 114 (1959) 1374.
5 Bozoki, G., E. Fenyves and L. Janossy, Nuclear Phys., 24 (1961) 412.
6 Alakoz, A. V., V. N. Bolotov, M. I. Devishev, L. F. Klimanova and A. P. Shmeleva, Canad. J. Phys., 46 (1968) 694.
7 Das, N. C., and M. S. Sinha, Bull. Natl. Inst. Sci. of India, 9 (1957) 80.
8 Rossi, B., High Energy Particles, Prentice Hall, New York (1952).
- Seitenbereich
-
0222 - 0224
- Zusammenfsg.
-
The production rate of nuclear interactions by neutral <I>N</I>-component of cosmic-rays of mean energy 15 GeV at sea level was studied as function of absorber thickness by means of a cloud chamber operated by coincidence and anticoincidence technique. The value of collision free path of non-ionizing <I>N</I>-rays in lead was found to be 232 ± 29 g/cm<sup>2</sup> and the collision cross-section 1.50 ± 0.19 bn. The estimated nucleon inelasticity for pion production in these interactions was 0.4.
- Artikel-Typen
- Kurzkommunikation