Has cosmological dark matter been observed?
Marcelo Salgado, Daniel Sudarsky, and Hernando Quevedo

TL;DR
This paper discusses evidence for dark matter in the universe, proposing a scalar field model that aligns with cosmological observations, galaxy distribution oscillations, and nucleosynthesis constraints, suggesting indirect detectability of dark matter.
Contribution
It introduces a scalar field model for dark matter that explains galaxy oscillations and fits cosmological and nucleosynthesis data, offering a new perspective on dark matter detection.
Findings
Scalar field model explains galaxy distribution oscillations
Model consistent with Big Bang nucleosynthesis constraints
Age of universe aligns with standard cosmological bounds
Abstract
There are many indications that ordinary matter represents only a tiny fraction of the matter content of the Universe, with the remainder assumed to consist of some different type of matter, which, for various reasons must be nonluminous (dark matter). Among these indications are the inflationary scenarios which predicts that the average energy density of the Universe coincides with the so called critical value (for which the expansion never stops but the rate of expansion approaches zero at very late times). At the same time it is known (from the predictions of Big Bang nucleosynthesis on the abundances of the light elements, other than Helium) that the baryonic energy density (ordinary matter) must represent ( \% (where is the Hubble constant in units of 100 km sMpc) of this critical value \cite{Copi,OstStein}. We present here evidence supporting…
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