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Cosmic ray $e^±$ at high energy
There is a commonly expressed opinion in the literature, that cosmic-ray (CR) e+ come from a primary source, which could be dark matter or pulsars. In these proceedings we review some evidence to the contrary: namely, that e+ come from secondary production due to CR nuclei scattering on interstellar...
| Autores principales: | , |
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| Lenguaje: | eng |
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2019
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| Acceso en línea: | https://dx.doi.org/10.1051/epjconf/201920804001 http://cds.cern.ch/record/2826890 |