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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...

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Detalles Bibliográficos
Autores principales: Bar, Nitsan, Blum, Kfir, Lacroix, Thomas, Panci, Paolo
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2019/07/045
http://cds.cern.ch/record/2676801