A closer look at the tertiary production of antiprotons in the Galaxy
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
Reference23 articles.
1. Cosmic Antiprotons as a Probe for Supersymmetric Dark Matter?
2. The Cosmic‐Ray Antiproton Flux between 0.62 and 3.19 GeV Measured Near Solar Minimum Activity
3. The Cosmic‐Ray Antiproton Flux between 3 and 49 GeV
4. Bogomolov, E.A., Lubyanaya, N.D., Romanov, V.A. In: Proceedings of the 16th International Cosmic Ray Conference (Kyoto), vol. 1, p. 330, 1979
5. Pion Production without Annihilation in Antiproton-Proton Interactions at 3.6 GeV/c
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Influence of microscopic particle interaction models on the flux of atmospheric antiprotons;Astroparticle Physics;2012-01
2. Study of low energy hadronic interaction models based on BESS observed cosmic ray proton and antiproton spectra at medium high altitude;Physical Review D;2009-06-23
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