This is a preview of subscription content, log in via an institution to check access.
References
R. P. Feynman andM. Gell-Mann:Phys. Rev.,109, 193 (1958).
T. Ericson andS. L. Glashow:Phys. Rev.,133, B 130 (1964).
G. Feinberg:Phys. Rev.,134, B 1295 (1964).
S. V. Pepper, C. Ryan, S. Okubo andR. E. Marshak:Phys. Rev.,137, B 1259 (1965).
B. D’Espagnat:Phys. Lett.,7, 204 (1963).
G. Bernardini, H. Bienlein, A. Böhm, G. von Dardel, H. Faissner, F. Ferrero, J.-M. Gaillard H. J. Gerber, B. Hahn, M. Holder, V. Kaftanov, F. Krienen, C. Manfredotti, M. Reinharz, R. A. Salmeron, A. Staude, H. J. Steiner, J. Bartley, M. M. Block, H. Burmeister, D. C. Cundy, D. Eiben, C. Franzinetti, J. Keren, R. Møllerud, G. Myatt, M. Nikolić, A. Orkin-Lecourtois, M. Paty, D. H. Perkins, C. A. Ramm, K. Schultze, H. Sletten, K. Soop, R. Stump, W. Venus andH. Yoshiki:Nuovo Cimento,38, 608 (1965).
R. Burns, K. Goulianos, E. Hyman, L. Lederman, W. Lee, N. Mistry, J. Rettberg, M. Schwartz, J. Sunderland andG. Danby:Phys. Rev. Lett.,15, 42 (1965).
S. Pakvasa, S. F. Tuan andT. T. Wu:Phys. Rev. Lett.,20, 1546 (1968).
C. G. Callan:Phys. Rev. Lett.,20, 809 (1968).
H. E. Bergeson, J. W. Keuffel, M. O. Larson, E. R. Martin andG. W. Mason:Phys. Rev. Lett.,19, 1487 (1967);21, 1089 (1968).
Our basic reasoning and conclusion agree withC. H. Woo:Phys. Rev. Lett.,21, 1419 (1968)
P. V. Ramana Murthy:Phys. Lett. 28 B, 38 (1968).
J. D. Bjorken, S. Pakvasa, W. Simmons andS. F. Tuan:Phys. Rev.,184, 1345 (1969).
J. B. Kogut:Phys. Rev.,186, 1540 (1969).
M. G. K. Menon, P. V. Ramana Murthy, B. V. Sreekanthan andS. Miyake:Phys. Lett. 5, 272 (1963).
F. Reines, M. F. Crouch, T. L. Jenkins, W. R. Kropp, H. S. Gurr, G. R. Smith, J. P. F. Sellschop andB. Meyer:Phys. Rev. Lett. 15, 429 (1965).
B. Pontecorvo:Žurn. Ėksp. Teor. Fiz.,37, 1751 (1959).
We use Feynman’s notation and conventions as described inR. P. Feynman:Theory of Fundamental Processes (New York, 1961).
S. Miyake, V. S. Narasimhan andP. V. Ramana Murthy:Nuovo Cimento,32, 1505 (1964).
R. Cowsik, Y. Pal andS. N. Tandon:Proc. Ind. Acad. Sci.,53, 217 (1966).
J. L. Osborne, S. S. Said andA. W. Wolfendale:Proc. Phys. Soc.,86, 93 (1965).
F. Reines:Proc. Roy. Soc., A301, 125 (1967).
M. G. K. Menons, and others:Proc. Roy. Soc. A301, 137 (1967).
I. Budagov, D. C. Cundy, C. Franzinetti, W. B. Fretter, H. W. K. Hopkins, C. Manfredotti, G. Myatt, F. A. Nezrick, M. Nikolić, T. B. Novey, R. B. Palmer, J. B. M. Pattison, D. H. Perkins, C. A. Ramm, B. Roe, R. Stump, W. Venus, H. W. Wachsmuth andH. Yoshiki:Phys. Lett.,30 B, 364 (1969).
R. E. Taylor:Proceedings of the International Conference on Electron and Photon Interactions at High Energy (Daresbury, 1969).
Several theoretical arguments have been advanced for a value of the W-mass below this limit,e. g. R. Marshak:Topical Conference on Weak Interactions (CERN, Geneva, 1969), p. 371.
Author information
Authors and Affiliations
Additional information
Address for 1970–71: University of Virginia, Charlottesville, Va.
Rights and permissions
About this article
Cite this article
Kabir, P.K., Kamal, A.N. Muon flux deep underground and the question of strong W-interactions. Lett. Nuovo Cimento 1, 1–8 (1971). https://doi.org/10.1007/BF02785035
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/BF02785035