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dc.creatorNaoz, Smadar-
dc.creatorLi, Gongjie-
dc.creatorZanardi, Macarena-
dc.creatorde Elia, Gonzalo Carlos-
dc.creatorDi Sisto, Romina Paula-
dc.date2018-11-16T17:44:48Z-
dc.date2018-11-16T17:44:48Z-
dc.date2017-07-
dc.date2018-10-22T19:51:54Z-
dc.date.accessioned2019-04-29T15:27:55Z-
dc.date.available2019-04-29T15:27:55Z-
dc.date.issued2018-11-16T17:44:48Z-
dc.date.issued2018-11-16T17:44:48Z-
dc.date.issued2017-07-
dc.date.issued2018-10-22T19:51:54Z-
dc.identifierNaoz, Smadar; Li, Gongjie; Zanardi, Macarena; de Elia, Gonzalo Carlos; Di Sisto, Romina Paula; The Eccentric Kozai-Lidov Mechanism for Outer Test Particle; IOP Publishing; Astronomical Journal; 154; 1; 7-2017; 1-11-
dc.identifier0004-6256-
dc.identifierhttp://hdl.handle.net/11336/64626-
dc.identifier1538-3881-
dc.identifierCONICET Digital-
dc.identifierCONICET-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/294639-
dc.descriptionThe secular approximation of the hierarchical three body systems has been proven to be very useful in addressing many astrophysical systems, from planets to stars to black holes. In such a system, two objects are on a tight orbit and the tertiary is on a much wider orbit. Here, we study the dynamics of a system by taking the tertiary mass to zero and solve the hierarchical three body system up to the octupole level of approximation. We find a rich dynamics that the outer orbit undergoes due to gravitational perturbations from the inner binary. The nominal result of the precession of the nodes is mostly limited for the lowest order of approximation; however, when the octupole level of approximation is introduced, the system becomes chaotic, as expected, and the tertiary oscillates below and above 90°, similarly to the non-test particle flip behavior. We provide the Hamiltonian of the system and investigate the dynamics of the system from the quadrupole to the octupole level of approximations. We also analyze the chaotic and quasi-periodic orbital evolution by studying the surfaces of sections. Furthermore, including general relativity, we showcase the long-term evolution of individual debris disk particles under the influence of a far-away interior eccentric planet. We show that this dynamics can naturally result in retrograde objects and a puffy disk after a long timescale evolution (a few Gyr) for initially aligned configuration.-
dc.descriptionFil: Naoz, Smadar. University of California; Estados Unidos. Mani L. Bhaumik Institute; Estados Unidos-
dc.descriptionFil: Li, Gongjie. Institute for Theory and Computation; Estados Unidos-
dc.descriptionFil: Zanardi, Macarena. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina-
dc.descriptionFil: de Elia, Gonzalo Carlos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina-
dc.descriptionFil: Di Sisto, Romina Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina-
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dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherIOP Publishing-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.3847/1538-3881/aa6fb0-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-3881/aa6fb0-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.subjectCELESTIAL MECHANICS-
dc.subjectCHAOS-
dc.subjectMINOR PLANETS, ASTEROIDS: GENERAL-
dc.subjectPLANETARY SYSTEMS-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleThe Eccentric Kozai-Lidov Mechanism for Outer Test Particle-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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