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Scalar Field Dark Matter as an Alternative Explanation for the Anisotropic Distribution of Satellite Galaxies by Solís-López, Jordi; Guzmán, Francisco S.; Matos, Tonatiuh; Robles, Victor H.; Ureña-López, L. Arturo is a scholarly article available to read on EtoBox.

What is Scalar Field Dark Matter as an Alternative Explanation for the Anisotropic Distribution of Satellite Galaxies about?

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

Author

Solís-López, Jordi; Guzmán, Francisco S.; Matos, Tonatiuh; Robles, Victor H.; Ureña-López, L. Arturo

Published

2019

Language

EN