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Looking for ultralight dark matter near supermassive black holes
Measurements of the dynamical environment of supermassive black holes (SMBHs) are becoming abundant and precise. We use such measurements to look for ultralight dark matter (ULDM), which is predicted to form dense cores (“solitons”) in the centre of galactic halos. We search for the gravitational im...
Autores principales: | Bar, Nitsan, Blum, Kfir, Lacroix, Thomas, Panci, Paolo |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2019/07/045 http://cds.cern.ch/record/2676801 |
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