paper

Supermassive dark-matter Q-balls in galactic centers?

arXiv:1510.07132 · doi:10.1088/1475-7516/2016/11/027

Abstract

Though widely accepted, it is not proven that supermassive compact objects (SMCOs) residing in galactic centers are black holes. In particular, the Milky Way's SMCO can be a giant nontopological soliton, Q-ball, made of a scalar field: this fits perfectly all observational data. Similar but tiny Q-balls produced in the early Universe may constitute, partly or fully, the dark matter. This picture explains in a natural way, why our SMCO has very low accretion rate and why the observed angular size of the corresponding radio source is much smaller than expected. Interactions between dark-matter Q-balls may explain how SMCOs were seeded in galaxies and resolve well-known problems of standard (non-interacting) dark matter.

15 pages (jcappub.sty), 3 figures. V2: clarifications and references added, version accepted by JCAP

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