| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1771021 | Astroparticle Physics | 2012 | 10 Pages |
Abstract
⺠The simulated antiproton flux depends strongly on particle interaction models. ⺠The knowledge of particle interaction characteristics is rather limited as yet. ⺠Prediction of galactic antiproton spectrum may consequently be quite uncertain. ⺠Interpretation of PAMELA results in terms of dark matter sources requires caution.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Arunava Bhadra, Biplab Bijay, Sanjay K. Ghosh, Partha S. Joarder, Sibaji Raha,