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Title: KINEMATICAL AND CHEMICAL VERTICAL STRUCTURE OF THE GALACTIC THICK DISK. II. A LACK OF DARK MATTER IN THE SOLAR NEIGHBORHOOD

Journal Article · · Astrophysical Journal
;  [1];  [2]
  1. Departamento de Astronomia, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile)
  2. European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago (Chile)

We estimated the dynamical surface mass density {Sigma} at the solar position between Z = 1.5 and 4 kpc from the Galactic plane, as inferred from the kinematics of thick disk stars. The formulation is exact within the limit of validity of a few basic assumptions. The resulting trend of {Sigma}(Z) matches the expectations of visible mass alone, and no dark component is required to account for the observations. We extrapolate a dark matter (DM) density in the solar neighborhood of 0 {+-} 1 mM{sub Sun} pc{sup -3}, and all the current models of a spherical DM halo are excluded at a confidence level higher than 4{sigma}. A detailed analysis reveals that a small amount of DM is allowed in the volume under study by the change of some input parameter or hypothesis, but not enough to match the expectations of the models, except under an exotic combination of non-standard assumptions. Identical results are obtained when repeating the calculation with kinematical measurements available in the literature. We demonstrate that a DM halo would be detected by our method, and therefore the results have no straightforward interpretation. Only the presence of a highly prolate (flattening q > 2) DM halo can be reconciled with the observations, but this is highly unlikely in {Lambda}CDM models. The results challenge the current understanding of the spatial distribution and nature of the Galactic DM. In particular, our results may indicate that any direct DM detection experiment is doomed to fail if the local density of the target particles is negligible.

OSTI ID:
22037261
Journal Information:
Astrophysical Journal, Vol. 751, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

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