Pico-charged intermediate particles rescue dark matter interpretation of 511 keV signal
Abstract Various alleged indirect dark matter search signals, such as the 511 keV line from galaxy center or the PAMELA/AMS02 signal, are often challenged by the absence of corresponding signal from dwarf galaxies and/or by the absence of an impact on CMB through delayed recombination. We propose a...
Tallennettuna:
| Päätekijät: | , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
SpringerOpen
2017-12-01
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| Sarja: | Journal of High Energy Physics |
| Aiheet: | |
| Linkit: | http://link.springer.com/article/10.1007/JHEP12(2017)083 |
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