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Scalar Field Wave Dark Matter and Galactic Halos.

Record Type:	Electronic resources : Monograph/item
Title/Author:	Scalar Field Wave Dark Matter and Galactic Halos./
Author:	Hamm, Benjamin.
Published:	Ann Arbor : ProQuest Dissertations & Theses, : 2021,
Description:	155 p.
Notes:	Source: Dissertations Abstracts International, Volume: 83-04, Section: B.
Contained By:	Dissertations Abstracts International83-04B.
Subject:	Astrophysics. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=28546527
ISBN:	9798460430826

Scalar Field Wave Dark Matter and Galactic Halos.
Hamm, Benjamin.

Scalar Field Wave Dark Matter and Galactic Halos. - Ann Arbor : ProQuest Dissertations & Theses, 2021 - 155 p.

Source: Dissertations Abstracts International, Volume: 83-04, Section: B.

Thesis (Ph.D.)--Duke University, 2021.

This item must not be sold to any third party vendors.

The question of ``What is Dark Matter?" has been a focus of cosmological research since the turn of the 20th century. Though the composition of Dark Matter is unknown, the existence of Dark Matter is crucial to the modern theory of cosmology. We focus on a theory of Dark Matter referred to as \extit{Scalar Field Wave Dark Matter} (SF$\\psi$DM), which has received an increasing amount of interest from the research community since the late 2000s. SF$\\psi$DM is a peculiar theory in which Dark Matter is composed of ultralight bosonic particles. As a result, SF$\\psi$DM has an astronomically large deBroglie wavelength, generating complicated wave dynamics on the largest cosmological scales. This thesis focuses on describing the status of SF$\\psi$DM theory, SF$\\psi$DM halos, and how SF$\\psi$DM halos are affected by the wave-like features of the scalar field. In particular, we offer an analysis of galactic rotation curves and how they relate to SF$\\psi$DM excited states. This analysis yields a novel model for an observed galactic trend referred to as the Baryonic Tully-Fisher Relation. Furthering this model, we formulate an eigenfunction decomposition which can be used to describe superpositions of excited states.

ISBN: 9798460430826Subjects--Topical Terms:

535904
Astrophysics.
Subjects--Index Terms:

Axions

Scalar Field Wave Dark Matter and Galactic Halos.
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245 1 0 $a Scalar Field Wave Dark Matter and Galactic Halos.
260 1 $a Ann Arbor : $b ProQuest Dissertations & Theses, $c 2021
300 $a 155 p.
500 $a Source: Dissertations Abstracts International, Volume: 83-04, Section: B.
500 $a Advisor: Bray, Hubert.
502 $a Thesis (Ph.D.)--Duke University, 2021.
506 $a This item must not be sold to any third party vendors.
520 $a The question of ``What is Dark Matter?" has been a focus of cosmological research since the turn of the 20th century. Though the composition of Dark Matter is unknown, the existence of Dark Matter is crucial to the modern theory of cosmology. We focus on a theory of Dark Matter referred to as \extit{Scalar Field Wave Dark Matter} (SF$\\psi$DM), which has received an increasing amount of interest from the research community since the late 2000s. SF$\\psi$DM is a peculiar theory in which Dark Matter is composed of ultralight bosonic particles. As a result, SF$\\psi$DM has an astronomically large deBroglie wavelength, generating complicated wave dynamics on the largest cosmological scales. This thesis focuses on describing the status of SF$\\psi$DM theory, SF$\\psi$DM halos, and how SF$\\psi$DM halos are affected by the wave-like features of the scalar field. In particular, we offer an analysis of galactic rotation curves and how they relate to SF$\\psi$DM excited states. This analysis yields a novel model for an observed galactic trend referred to as the Baryonic Tully-Fisher Relation. Furthering this model, we formulate an eigenfunction decomposition which can be used to describe superpositions of excited states.
590 $a School code: 0066.
650 4 $a Astrophysics. $3 535904
650 4 $a Theoretical physics. $3 2144760
650 4 $a Physics. $3 516296
653 $a Axions
653 $a Dark Matter
653 $a Galaxies
653 $a General Relativity
653 $a Scalar Field
690 $a 0596
690 $a 0753
690 $a 0605
710 2 $a Duke University. $b Physics. $3 1035984
773 0 $t Dissertations Abstracts International $g 83-04B.
790 $a 0066
791 $a Ph.D.
792 $a 2021
793 $a English
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=28546527