Abstract
In this talk I discuss two problems in high energy particle astrophysics, the flux of cosmic ray antiprotons and the chemical composition in the region of the ‘‘knee’’ of the cosmic ray energy spectrum (∼1015 eV). Both are rather poorly known at present, yet they have great potential for informing us about the sources, acceleration and propagation of high energy cosmic radiation.
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.
