Dynamical evidence of a dark solitonic core of 109M⊙ in the milky way

A 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 Schrodinger-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, similar or equal to 100 pc, of mass similar or equal to 10(9)M(circle dot). 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 similar or equal to 130 km/s, corresponding to an excess central mass of similar or equal to 1.5x10(9)M(circle dot) within similar or equal to 100 pc, favoring a boson mass of similar or equal to 10(-22) eV. 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. (C) 2020 Elsevier B.V. All rights reserved.