De Martino I.Broadhurst, T.T.BroadhurstHenry Tye, S.-H.S.-H.Henry TyeChiueh, T.T.ChiuehHSI-YU SCHIVE2021-07-282021-07-28202022126864https://www.scopus.com/inward/record.uri?eid=2-s2.0-85079381597&doi=10.1016%2fj.dark.2020.100503&partnerID=40&md5=62d13df95797305efa3c1faca74ea23ehttps://scholars.lib.ntu.edu.tw/handle/123456789/575294A wavelike solution for the non-relativistic universal dark matter (wave-DM) is rapidly gaining interest, following pioneering simulations of cosmic structure as an interference pattern of coherently oscillating bosons. A prominent solitonic standing wave is predicted at the center of every galaxy, representing the ground state solution of the coupled Schr?dinger–Poisson equations, and it has been identified with the wide, kpc scale dark cores of common dwarf-spheroidal galaxies. A denser soliton is predicted for Milky Way sized galaxies where momentum is higher, so the de Broglie scale of the soliton is smaller, ?100 pc, of mass ?109M⊙. Here we show the central motion of bulge stars in the Milky Way implies the presence of such a dark core, where the velocity dispersion rises inversely with radius to a maximum of ?130 km/s, corresponding to an excess central mass of ?1.5×109M⊙ within ?100 pc, favoring a boson mass of ?10?22eV. This quantitative agreement with such a unique and distinctive prediction is therefore strong evidence for a light bosonic solution to the long standing Dark Matter puzzle. ? 2020 Elsevier B.V.journal article10.1016/j.dark.2020.1005032-s2.0-85079381597