No evidence of dark matter in the solar neighborhood
C. Moni Bidin, G. Carraro, R. A. Mendez, R. Smith

TL;DR
This study measures the mass density near the Sun and finds no evidence of dark matter in that region, challenging existing dark matter models unless assuming an unlikely halo shape.
Contribution
It provides direct kinematic measurements showing the absence of dark matter in the solar neighborhood, contradicting standard dark matter halo models.
Findings
No dark matter detected in the solar neighborhood
Current dark matter halo models are statistically excluded
Results suggest a need to revise dark matter distribution models
Abstract
We measured the surface mass density of the Galactic disk at the solar position, up to 4 kpc from the plane,by means of the kinematics of ~400 thick disk stars. The results match the expectations for the visible mass only, and no dark matter is detected in the volume under analysis. The current models of dark matter halo are excluded with a significance higher than 5sigma, unless a highly prolate halo is assumed, very atypical in cold dark matter simulations. The resulting lack of dark matter at the solar position challenges the current models.
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation
