Scalar field dark matter as an alternative explanation for the anisotropic distribution of satellite galaxies

Abstract

In recent years, the scalar field dark matter (SFDM), also called ultralight bosonic dark matter, has received considerable attention due to the number of problems it might help to solve. Among these are the cusp-core problem and the abundance of small structures of the standard cold dark matter (CDM) model. In this paper we show that multi-state solutions of the low energy and weak gravitational field limit of field equations, interpreted as galactic halo density profiles, can provide a possible explanation to the anisotropic distribution of satellite galaxies observed in the Milky Way, M31 and Centaurus A, where satellites trajectories seem to concentrate on planes close to the poles of the galaxies instead of following homogeneously distributed trajectories. The core hypothesis is that multi-state solutions of the equations describing the dynamics of this dark matter candidate, namely, the Gross-Pitaevskii-Poisson equations, with monopolar and dipolar contributions, can possibly explain the anisotropy of satellite trajectories. In order to construct a proof of concept, we study the trajectories of a number of test particles traveling on top of the gravitational potential due to a multi-state halo with modes (1,0,0)+(2,1,0). The result is that particles accumulate asymptotically in time on planes passing close to the poles. Satellite galaxies are not test particles but interpreted as such, our results indicate that in the asymptotic time their trajectories do not distribute isotropically, instead they prefer to have orbital poles accumulating near the equatorial plane of the multistate halo. The concentration of orbital poles depends on whether the potential is monopolar or dipolar dominated.

This version has been accepted for publication in Physical Review D

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Cited by in corpus (12)

• Short Review of the main achievements of the Scalar Field, Fuzzy, Ultralight, Wave, BEC Dark Matter model
• Schrödinger-Poisson Solitons: Perturbation Theory
• Constraining Self-interacting Scalar Field Dark Matter From the Black Hole Shadow of the Event Horizon Telescope
• Probing dark matter with polarimetry techniques
• Analyzing Planar Galactic Halo Distributions with Fuzzy/Cold Dark Matter Models
• The quantum character of the Scalar Field Dark Matter
• Theory and phenomenology of stressed wave-dark-matter soliton
• Dark sector domain walls could explain the observed planes of satellites
• Possible formation mechanism of multistate gravitational atoms
• A Natural Explanation of the VPOS from Multistate Scalar Field Dark Matter
• Equilibrium Core and Vortex Solutions of Bose Einstein Condensate Dark Matter around a Black Hole
• Constraining Light Scalar Field with Torsion-Balance Gravity Experiments