Published September 2021 | Version v1
Journal article

Implications of triangular features in the Gaia skymap for the Caustic Ring Model of the Milky Way halo

  • 1. Department of Physics, University of Florida, Gainesville, FL 32611 (United States)
  • 2. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Torino, Via P. Giuria 1, I-10125 Torino (Italy)
  • 3. Dipartimento di Fisica, Università di Torino, Via P. Giuria 1, I-10125 Torino (Italy)
  • 4. Department of Astronomy, University of Florida, Gainesville, FL 32611 (United States)

Description

The Gaia map of the Milky Way reveals a pair of triangular features at nearly symmetric locations on opposite sides of the Galactic Center. In this paper we explore the implications of these features assuming they are manifestations of a caustic ring in the dark matter distribution of the Milky Way halo. The existence of a series of such rings is predicted by the Caustic Ring Model. The model's phase-space distribution is that acquired by a rethermalizing Bose–Einstein condensate of axions or axion-like particles. We show that dust is gravitationally entrained by cold axion flows and propose this as an explanation for the sharpness of the triangular features. The locations of the features imply that we on Earth are much closer to the fifth caustic ring than thought on the basis of pre-Gaia observations. Most likely we are inside its tricusp cross-section. In that case the dark matter density on Earth is dominated by four cold flows, termed Big, Little, Up and Down. If we are outside the tricusp cross-section the dark matter density on Earth is dominated by two cold flows, Big and Little. We use the triangular features in the Gaia map, and a matching feature in the IRAS map, to estimate the velocity vectors and densities of the four locally dominant flows.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.dark.2021.100838

Additional details

Identifiers

DOI
10.1016/j.dark.2021.100838;
PII
S2212686421000698;

Publishing Information

Journal Title
Physics of the Dark Universe
Journal Volume
33
Journal Page Range
vp.
ISSN
2212-6864

Optional Information

Copyright
Copyright (c) 2021 Elsevier B.V. All rights reserved.