Decaying Dark Atom Constituents and Cosmic Positron Excess
We present a scenario where dark matter is in the form of dark atoms that can accommodate the experimentally observed excess of positrons in PAMELA and AMS-02 while being compatible with the constraints imposed on the gamma-ray ux from Fermi/LAT. This scenario assumes that the dominant component of...
| Huvudupphovsmän: | , , , |
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| Materialtyp: | Artikel |
| Språk: | English |
| Publicerad: |
Hindawi Limited
2014-01-01
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| Serie: | Advances in High Energy Physics |
| Länkar: | http://dx.doi.org/10.1155/2014/214258 |