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- W3100597821 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." @default.
- W3100597821 created "2020-11-23" @default.
- W3100597821 creator A5089715845 @default.
- W3100597821 date "2016-11-11" @default.
- W3100597821 modified "2023-09-23" @default.
- W3100597821 title "Supermassive dark-matter Q-balls in galactic centers?" @default.
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- W3100597821 doi "https://doi.org/10.1088/1475-7516/2016/11/027" @default.
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