Dark Matter in Cosmology
Vladimir Lukovic, Paolo Cabella, Nicola Vittorio

TL;DR
This paper reviews the progress in understanding dark matter in cosmology, covering theoretical models, experimental constraints, and key evidence like the Bullet cluster, highlighting advances from local surveys to cosmological data.
Contribution
It provides a comprehensive overview of dark matter research, integrating methods and recent data to strengthen the evidence for dark matter's existence and properties.
Findings
Stringent constraints on dark matter properties from cosmological data
Multiple methods converge to support dark matter's existence
Key evidence like the Bullet cluster confirms dark matter presence
Abstract
In this paper we review the main theoretical and experimental achievements in the field of Dark Matter from the Cosmological and Astrophysical point of view. We revisit it from the very first surveys of local astrophysical matter, up to the stringent constraints on matter properties, coming from the last release of data on cosmological scales. To bring closer and justify the idea of dark matter, we will go across methods and tools for measuring dark matter characteristics, and in some cases a combination of methods that provide one of the greatest direct proofs for dark matter, such as Bullet cluster.
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