The role of galaxy formation in the structure and dynamics of dark matter halos
Chiara Tonini

TL;DR
This paper explores how galaxy formation influences the structure and dynamics of dark matter halos, emphasizing the joint evolution of baryonic matter and dark matter during galaxy formation.
Contribution
It proposes that galaxy formation perturbs halo equilibrium, leading to evolving configurations, and highlights the importance of coupled baryonic and dark matter evolution.
Findings
Baryonic collapse perturbs halo equilibrium
Dark matter halos are sensitive to inner dynamical perturbations
Halo and galaxy properties are linked through joint evolution
Abstract
The structure and dynamics of dark matter halos, as predicted by the hierarchical clustering scenario, are at odds with the properties inferred from the observations at galactic scales. My Thesis addresses this problem by taking an evolutionary approach. I analysed in detail the many and different observational evidences of a discrepancy the predicted halo equilibrium state and the one inferred from the measurable properties of disk galaxies, as well as of the scaling relations existing between the angular momentum, geometry and mass distribution of the luminous and dark components, and realized that they all seem to point towards the same conclusion: the baryons hosted inside the halo, by collapsing and assembling to form the galaxy, perturb the halo equilibrium structure and made it evolve into new configurations. From the theoretical point of view, the behaviour of dark matter halos…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies
