인문학
사회과학
자연과학
공학
의약학
농수해양학
예술체육학
복합학
DBpia AI
AI 에이전트
AI 아이디어
AI 리더
AI 뷰어
Citeasy
크롬 서지관리 다운로드
지원사업
학술연구/단체지원/교육 등 연구자 활동을 지속하도록 DBpia가 지원하고 있어요.
커뮤니티
연구자들이 자신의 연구와 전문성을 널리 알리고, 새로운 협력의 기회를 만들 수 있는 네트워킹 공간이에요.
초록·키워드
The von Zeipel-Lidov-Kozai (ZLK) effect has been applied to a wide range of dynamical circumstances, covering satellites and planets to supermassive black holes, in order to explain physical phenomena. The evolution of periodic orbit families associated with ZLK resonance under the octupole-level approximation exhibits distinctly different dynamical structures from the standard ZLK effect. In particular, bifurcations of periodic-orbit families commonly exist in planetary systems with a wide range of mass ratios. It is shown that such a phenomenon of bifurcation is triggered by ZLK secondary resonance, which is a new dynamical mechanism that has not appeared in previous studies. Numerical analysis shows that ZLK secondary resonance leads to a stronger excitation of eccentricity and/or inclination than the standard ZLK effect and that the level of enhancement is dependent on the initial eccentricity. The technique of perturbative treatments is adopted to study dynamical structures of ZLK secondary resonances, showing that there is an excellent agreement between analytical structures arising in phase portraits and numerical structures arising in Poincaré sections. Phase-space structures are produced for actual exoplanetary systems including HAT-P-11, HAT-P-13, and HAT-P-44, where large excitation of planetary eccentricity and/or inclination is expected due to the emergence of ZLK secondary resonance.
인공지능 문자 인식 모델을 통해 추출된 텍스트로, 일부 오타나 오류가 포함될 수 있으나 지속적으로 개선 중입니다.
오류를 발견하셨다면 해당 부분을 드래그한 후 ' 를 통해 신고해주세요.
오류를 발견하셨다면 해당 부분을 드래그한 후 ' 를 통해 신고해주세요.
최근 본 자료 전체보기
