Stars Initiated by High Energy Protons and Neutrons
- 15 April 1952
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 86 (2) , 167-170
- https://doi.org/10.1103/PhysRev.86.167
Abstract
Stars initiated in nuclear emulsions by 240-Mev protons and 180-Mev neutrons have been studied. Size-frequency distributions of the stars and angular distributions of prongs in various energy intervals have been obtained. Comparison with similar results obtained at different energies shows that the star size distribution is more sensitive to incident energy for protons than for neutrons.Keywords
This publication has 9 references indexed in Scilit:
- Experiments on Proton-Proton Scattering from 120 to 345 MevPhysical Review B, 1951
- On the Goldberger Model for the Interaction of High Energy Nucleons with Heavy NucleiPhysical Review B, 1951
- Stars in Photographic Emulsions Initiated by ProtonsPhysical Review B, 1951
- Variation with Energy of Nuclear Collision Cross Sections for High Energy NeutronsPhysical Review B, 1951
- Stars produced in nuclear emulsions by 150 MeV. neutronsJournal of Computers in Education, 1951
- Stars Induced by 350- to 400-Mev ProtonsPhysical Review B, 1950
- Proton-Proton Scattering at 100 MevPhysical Review B, 1950
- Stars in Photographic Emulsions Initiated by Alpha-ParticlesPhysical Review B, 1949
- Stars in Photographic Emulsions Initiated by Deuterons. Part I. ExperimentalPhysical Review B, 1949