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Dynamical Evidence of a Solitonic Core of $10^{9}M_\odot$ in the Milky Way

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arxiv 1807.08153 v3 pith:O2SAQY5R submitted 2018-07-21 astro-ph.GA gr-qchep-th

classification astro-ph.GAgr-qchep-th
keywords simeqdarkmassmilkyodotbosoncentralcore
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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, $\simeq 10^{-22}$ 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, $\simeq 100$ pc, of mass $\simeq 10^9 M_\odot$. 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 $\simeq 130$ km/s, corresponding to an excess central mass of $\simeq 1.5\times 10^9 M_\odot$ within $\simeq 100$ pc, favouring a boson mass of $\simeq 10^{-22}$ 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, such as the axions generic in String Theory.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Fuzzy Dark Matter Soliton Cores around Supermassive Black Holes

    astro-ph.GA 2019-08 conditional novelty 4.0 of 10

    A supermassive black hole perturber squeezes fuzzy dark matter soliton cores toward hydrogen-atom-like profiles, and M87 observations forbid FDM particle masses near 10^-22 eV.

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