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Dynamical Evolution of Multi-Orbiter Systems: Applications to Planets, Protoplanetary Disks, and Black Holes- [electronic resource]
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Dynamical Evolution of Multi-Orbiter Systems: Applications to Planets, Protoplanetary Disks, and Black Holes- [electronic resource]
자료유형  
 학위논문
Control Number  
0016932497
International Standard Book Number  
9798380314817
Dewey Decimal Classification Number  
520
Main Entry-Personal Name  
Li, Jiaru.
Publication, Distribution, etc. (Imprint  
[S.l.] : Cornell University., 2023
Publication, Distribution, etc. (Imprint  
Ann Arbor : ProQuest Dissertations & Theses, 2023
Physical Description  
1 online resource(298 p.)
General Note  
Source: Dissertations Abstracts International, Volume: 85-03, Section: B.
General Note  
Advisor: Lai, Dong.
Dissertation Note  
Thesis (Ph.D.)--Cornell University, 2023.
Restrictions on Access Note  
This item must not be sold to any third party vendors.
Summary, Etc.  
요약Systems with massive central objects and multiple smaller orbiters appear in many astrophysical contexts. Their dynamical evolution cannot be described by analytic solutions with finite numbers of terms except for some special cases. In this dissertation, I use semi-analytical methods, N-body simulations, and hydrodynamics simulations to study the dynamical evolution in different kinds of multi-orbiter scenarios: (i) I investigate the outcomes of dynamical instability in planetary systems. I incorporate hydrodynamics effects during planet-planet close encounters into long-term numerical integration, and present the resulting distributions of planetary orbital eccentricities, spins, and obliquities. (ii) I show that, under certain conditions, self-gravitating protoplanetary disks around stars may be prone to a new hydrodynamical instability called eccentric mode instability (EMI). This instability causes disks to develop coherent eccentric patterns spontaneously. I then examine a new way to form rings in disks via EMI, and find a new mechanism to produce highly eccentric exoplanets through a secular resonance between planets and eccentric disks. (iii) I explore the dynamics of stellar-mass black holes (BHs) embedded in gaseous accretion disks around supermassive BHs. I show that these embedded BHs may form long-lived binaries through close encounters due to either gravitational wave emission or gas drag.
Subject Added Entry-Topical Term  
Astronomy.
Subject Added Entry-Topical Term  
Astrophysics.
Subject Added Entry-Topical Term  
Planetology.
Index Term-Uncontrolled  
Black holes
Index Term-Uncontrolled  
Exoplanets
Index Term-Uncontrolled  
Gravitational wave sources
Index Term-Uncontrolled  
Hydrodynamics
Index Term-Uncontrolled  
Protoplanetary disks
Added Entry-Corporate Name  
Cornell University Astronomy and Space Sciences
Host Item Entry  
Dissertations Abstracts International. 85-03B.
Host Item Entry  
Dissertation Abstract International
Electronic Location and Access  
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Control Number  
joongbu:642972
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