Abstract

Nucleus-nucleus interactions produced by heavy cosmic ray primaries in nuclear emulsions have been analysed. The kinetic energy of the incident nuclei is 100-500 MeV/nucleon. Whenever possible the particles leaving the point of interaction have been identified and their emission angles and kinetic energies have been measured. The angular and energy distribution of the protons emitted can be understood if reasonable values of the momenta of the interacting nucleons inside the colliding nuclei are considered, and if it is further assumed that interactions between nucleons and clusters of nucleons occur. The momentum distribution of the emitted protons and alpha-particles is consistent with an average recoil momentum of the target nuclei of about 23 MeV/c per nucleon. It is found that about 30% of the particles with ranges in the interval 10 μm<R<100 μm cannot be explained by ordinary evaporation theory. The spallation of the target and the projectile has been studied. It was found that the disintegration of the two interacting nuclei increases with increasing projectile energy.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.