Detection of a universal core-halo transition in dwarf galaxies as predicted by Bose-Einstein dark matter
Alvaro Pozo, Tom Broadhurst, Ivan de Martino, Tzihong Chiueh, George, F. Smoot, Silvia Bonoli, Raul Angulo

TL;DR
This paper provides evidence for a universal core-halo transition in dwarf galaxies consistent with Bose-Einstein dark matter, revealing a distinctive density profile that supports the light boson model over traditional heavy particle dark matter.
Contribution
It identifies the predicted core-halo structure in dwarf galaxies' stellar profiles, supporting Bose-Einstein dark matter and explaining observed features including tidal stripping effects.
Findings
Detection of a density transition at ~1 kpc in isolated dwarfs.
Larger density transitions in Milky Way satellites imply tidal stripping.
Supports light boson dark matter model over heavy particle scenarios.
Abstract
The presence of large dark matter cores in dwarf galaxies has long been puzzling and many are now known to be surrounded by an extensive halo of stars. Distinctive core-halo structure is characteristic of dark matter as a Bose Einstein condensate, DM, with a dense, soliton core predicted in every galaxy, representing the ground state, surrounded by a large, tenuous halo of excited density waves. A marked density transition is predicted between the core and the halo set by the de Broglie wavelength, as the soliton core is a prominent standing wave that is denser by over an order of magnitude than the surrounding halo. Here we identify this predicted behavior in the stellar profiles of the well known "isolated" dwarfs that lie outside the Milky Way, each with a clear density transition at , implying a very light boson, eV. The…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
