서브메뉴
검색
Dynamical Evolution of Multi-Orbiter Systems: Applications to Planets, Protoplanetary Disks, and Black Holes- [electronic resource]
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
- 로그인을 한후 보실 수 있는 자료입니다.
- Control Number
- joongbu:642972
Buch Status
- Reservierung
- 캠퍼스간 도서대출
- 서가에 없는 책 신고
- Meine Mappe