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Self-Interacting Dark Matter Subhalos and Dwarf Satellite Galaxies: Evolution and Diversity.
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Self-Interacting Dark Matter Subhalos and Dwarf Satellite Galaxies: Evolution and Diversity.
자료유형  
 학위논문
Control Number  
0017165024
International Standard Book Number  
9798384462385
Dewey Decimal Classification Number  
523
Main Entry-Personal Name  
Zeng, Zhichao Carton.
Publication, Distribution, etc. (Imprint  
[S.l.] : The Ohio State University., 2024
Publication, Distribution, etc. (Imprint  
Ann Arbor : ProQuest Dissertations & Theses, 2024
Physical Description  
275 p.
General Note  
Source: Dissertations Abstracts International, Volume: 86-04, Section: B.
General Note  
Advisor: Peter, Annika.
Dissertation Note  
Thesis (Ph.D.)--The Ohio State University, 2024.
Summary, Etc.  
요약Self-interacting dark matter (SIDM) cosmologies admit an enormous diversity of dark matter (DM) halo density profiles, from low-density cores to high-density core-collapsed cusps. The possibility of the growth of high central density in low-mass halos, accelerated if halos are subhalos of larger systems, has intriguing consequences for small-scale observables such as substructure lensing, dwarf galaxies and stellar streams. However, following the evolution of low-mass subhalos in their host systems is computationally expensive, sometimes even prohibitive, with traditional N-body cosmological simulations. In this thesis work, we are thus motivated to develop a series of hybrid methods for simulations of low-mass subhalos, from core-creation to core-collapse (or complete dissolution in the host), also with the orbital effects from the host halo consistently captured. This thesis consists of three parts: in the first chapter, we detail our hybrid method tracing individual SIDM subhalos; in the second chapter, we use the hybrid method to simulate a realistic population of subhalos, also with a new hierarchical framework to further reduce the computational cost; in the third chapter, we populate individual SIDM subhalos with galaxies in the initial condition, and study the evolution of stellar properties in response to SIDM halo evolution and orbital effects.
Subject Added Entry-Topical Term  
Astrophysics.
Subject Added Entry-Topical Term  
Physics.
Subject Added Entry-Topical Term  
Applied physics.
Index Term-Uncontrolled  
Dark matter
Index Term-Uncontrolled  
Dwarf galaxy diversity
Index Term-Uncontrolled  
Substructure lensing
Index Term-Uncontrolled  
N-body simulation
Added Entry-Corporate Name  
The Ohio State University Physics
Host Item Entry  
Dissertations Abstracts International. 86-04B.
Electronic Location and Access  
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Control Number  
joongbu:658510
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