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Antiprotons in CR: What Do They Tell Us?
| Content Provider | Semantic Scholar |
|---|---|
| Author | Moskalenko, Igor V. Strong, Andrew Mashnik, Stepan G. Ormes, Jonathan F. |
| Copyright Year | 2003 |
| Abstract | Recent measurements of the CR ¯ p flux have been shown to pose a problem for conventional propagation models. In particular, models consistent with secondary/primary nuclei ratio in CR produce too few ¯ p’s, while matching the ratio and the ¯ p flux requires ad hoc assumptions. This may indicate an additional local CR component or new phenomena in CR propagation in the Galaxy. We discuss several possibilities which may cause this problem. |
| Starting Page | 1921 |
| Ending Page | 1924 |
| Page Count | 4 |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://arxiv.org/pdf/astro-ph/0306368v1.pdf |
| Alternate Webpage(s) | https://web.stanford.edu/~imos/papers/2003icrc....4.1921M.pdf |
| Alternate Webpage(s) | https://arxiv.org/pdf/astro-ph/0306368v1.pdf |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |
