Dynamical constraints on the galaxy-halo connection

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Abstract/Contents

Abstract
Dark matter halos comprise the bulk of the universe's mass, yet must be probed by the luminous galaxies that form within them. A key goal of modern astrophysics is to robustly relate the visible and dark mass, which to first order means relating the properties of galaxies and halos. The aim of this thesis is to develop and evaluate models of the galaxy-halo connection using observations of galaxy dynamics. In particular, I build empirical models based on the technique of halo abundance matching for five key dynamical scaling relations of galaxies -- the Tully-Fisher, Faber-Jackson, mass-size and mass discrepancy-acceleration relations, and Fundamental Plane -- which relate their baryon distributions and rotation or velocity dispersion profiles. I then develop a statistical scheme based on approximate Bayesian computation to compare the predicted and measured values of a number of summary statistics describing the relations' important features. I find some features to be naturally accounted for by an abundance matching approach and others to impose new constraints on the galaxy-halo connection; the remainder are challenging to reproduce and may imply galaxy-halo correlations beyond the scope of basic abundance matching. Besides providing concrete statistical tests of specific galaxy formation theories, these results will be of use for guiding the inputs of empirical and semi-analytic galaxy formation models, which require galaxy-halo correlations to be imposed by hand.

Description

Type of resource text
Form electronic; electronic resource; remote
Extent 1 online resource.
Publication date 2017
Issuance monographic
Language English

Creators/Contributors

Associated with Desmond, Harry
Associated with Stanford University, Department of Physics.
Primary advisor Wechsler, Risa H. (Risa Heyrman)
Thesis advisor Wechsler, Risa H. (Risa Heyrman)
Thesis advisor Abel, Tom G, 1970-
Thesis advisor Blandford, Roger D
Advisor Abel, Tom G, 1970-
Advisor Blandford, Roger D

Subjects

Genre Theses

Bibliographic information

Statement of responsibility Harry Desmond.
Note Submitted to the Department of Physics.
Thesis Thesis (Ph.D.)--Stanford University, 2017.
Location electronic resource

Access conditions

Copyright
© 2017 by Harry F. Desmond
License
This work is licensed under a Creative Commons Attribution Non Commercial 3.0 Unported license (CC BY-NC).

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