Impact of uncertainties in the halo velocity profile on direct detection of sub-GeV dark matter
Abstract We use the state-of-the-art high-resolution cosmological simulations by IllustrisTNG to derive the velocity distribution and local density of dark matter in galaxies like our Milky Way and find a substantial spread in both quantities. Next we use our findings to examine the sensitivity to t...
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| Hlavní autoři: | , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
SpringerOpen
2020-07-01
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| Edice: | Journal of High Energy Physics |
| Témata: | |
| On-line přístup: | http://link.springer.com/article/10.1007/JHEP07(2020)081 |
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