Dynamical Evidence of a Solitonic Core of $10^{9}M_\odot$ in the Milky Way
Ivan De Martino, Tom Broadhurst, S.-H. Henry Tye, Tzihong Chiueh,, Hsi-Yu Schive

TL;DR
This paper provides evidence for a solitonic dark matter core in the Milky Way, consistent with wave-DM models predicting a dense bosonic core of about 10^9 solar masses within 100 parsecs.
Contribution
It presents observational evidence supporting the existence of a solitonic dark matter core in the Milky Way, aligning with wave-DM theoretical predictions.
Findings
Central star velocity dispersion peaks at ~130 km/s
Excess mass of ~1.5×10^9 solar masses within 100 pc
Supports boson mass of ~10^{-22} eV
Abstract
A wavelike solution for the non-relativistic universal dark matter (wave-DM) is rapidly gaining interest, following distinctive predictions of 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, that has been identified with the wide, kpc scale dark cores of common dwarf-spheroidal galaxies, providing a boson mass of, eV. A denser soliton is predicted for Milky Way sized galaxies where momentum is higher, so the de Broglie scale of the soliton is smaller, pc, of mass . 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 km/s,…
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