25 pp.
25 pp.
| 715 K 25 pp. | |
| View Document | ||
| Title | Intensity of Upward Muon Flux Due to Cosmic-Ray Neutrinos Produced in the Atmosphere | |
| Author(s) | Lee, T. D.; Robinson, H.; Schwartz, M.; Cool, R. | |
| Publication Date | June 1963 | |
| Report Number | NEVIS-115 | |
| Unique Identifier | ACC0343 | |
| Other Numbers | OSTI ID: 4685861 | |
| Research Org | Columbia University, Irvington-on-Hudson, N.Y. Nevis Cyclotron Laboratory | |
| Contract No | AT(30-1)-1932 | |
| Sponsoring Org | U.S. Atomic Energy Commission (AEC) | |
| Subject | Physics; Atmosphere; Bosons; Cosmic Radiation; Elementary Particles; Energy Range; Field Theory; Interactions; Intermediate Boson; Muons; Neutrinos; Numericals; Production | |
| Related Web Pages | Melvin Schwartz and the Discovery of the Muon Neutrino | |
| Abstract | Calculations were performed to determine the upward going muon flux leaving the earth's surface after production by cosmic-ray neutrinos in the crust. Only neutrinos produced in the earth's atmosphere are considered. Rates of the order of one per 100 sq m/day might be expected if an intermediate boson exists and has a mass less than 2 Bev. (auth) | |
| 715 K 25 pp. | |
| View Document | ||
