Abstract
We reassess the problem of the production of the light elements lithium, beryllium, and boron, by energetic collisions between Galactic cosmic rays (GCR) and interstellar gas nuclei, in the framework of a consistent model for the chemical evolution of our Galaxy. We propose a new scenario for the propagation of GCR in the early Galaxy suggesting that, during its halo phase, GCR were more efficiently confined than today and had flatter spectra at low 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 callDisclaimer: 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.
