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Ultra-heavy cosmic-ray science--Are r-process nuclei in the cosmic rays produced in supernovae or binary neutron star mergers?

W. R. Binns,M. H. Israel,B. F. Rauch,A. C. Cummings,A. J. Davis,A. W. Labrador,R. A. Leske,R. A Mewaldt,E. C. Stone,M. E. Wiedenbeck,T. J. Brandt,E. R. Christian,J. T. Link,J. W. Mitchell,G. A. de Nolfo,T. T. von Rosenvinge,K. Sakai,M. Sasaki,C. J. Waddington,H. T. Janka,A. L. Melott,G. M. Mason,E-S. Seo,J. H. Adams,F-K. Thielemann,A. Heger, M. Lugaro,A. J. Westphal

arXiv: High Energy Astrophysical Phenomena（2019）

Cited 3|Views12
Key words
binary neutron star mergers,cosmic-ray rays,supernovae,ultra-heavy,r-process
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