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
References in corpus (21)
- A luminous quasar at a redshift of z = 7.085
- Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
- Shadows of Kerr black holes with scalar hair
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- An Unambiguous Detection of Faraday Rotation in Sagittarius A*
- An Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis
- Supermassive Black Holes from Ultra-Strongly Self-Interacting Dark Matter
- Kerr black holes with self-interacting scalar hair: hairier but not heavier
- Radio and Millimeter Monitoring of Sgr A*: Spectrum, Variability, and Constraints on the G2 Encounter
- The Galactic Center cloud G2 and its gas streamer
- Magnon condensation into Q-ball in 3He-B
- Event-Horizon-Telescope Evidence for Alignment of the Black Hole in the Center of the Milky Way with the Inner Stellar Disk
- Gravitational waves from fragmentation of a primordial scalar condensate into Q-balls
- Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
- How does gravity save or kill Q-balls?
- Gravitational waves from Affleck-Dine condensate fragmentation
- IceCube potential for detecting Q-ball dark matter in gauge mediation
- No asymmetric outflows from Sagittarius A* during the pericenter passage of the gas cloud G2
- No Microwave Flare of Sagittarius A* around the G2 Periastron Passing
Cited by in corpus (15)
- Boson Stars and Oscillatons: A Review
- Review of non-topological solitons in theories with -symmetry
- Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars
- Rn emanation measurements for the XENON1T experiment
- Propagation of self-localised Q-ball solitons in the He universe
- The fate of small classically stable Q-balls
- Non-topological solitons and quasi-solitons
- Magnon Bose-Einstein condensates: from time crystals and quantum chromodynamics to vortex sensing and cosmology
- Quasi-Compact Q-Balls
- Weyl-Invariant Gravity and the Nature of Dark Matter
- Hydrodynamic and Rayleigh-Plateau instabilities of Q-strings
- The Resurgence of the G(2) Group for the Strong Sector and the Emergence of Dark Matter
- Can dark-matter Q-balls grow to the mass gap masses?
- Soliton boson stars, Q-balls and the causal Buchdahl bound
- Understanding the Quantized Angular Momentum of Rotating Q-balls