The 3.5 keV line from stringy axions
Abstract An interesting result in particle astrophysics is the recent detection of an unexplained 3.5 keV line from galaxy clusters. A promising model, which can explain the morphology of the signal and its non-observation in dwarf spheroidal galaxies, involves a 7keV dark matter particle decaying i...
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| Glavni autori: | , , , |
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| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
SpringerOpen
2017-10-01
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| Serija: | Journal of High Energy Physics |
| Teme: | |
| Online pristup: | http://link.springer.com/article/10.1007/JHEP10(2017)192 |
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