CV Lattes
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Universidade Federal do ABC (UFABC). Centro de Ciências Naturais e Humanas (CCNH) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Bachelor's in Physics from Universidade Estadual de Campinas (UNICAMP, 2008), Master's in Mathematics from UNICAMP (2010) and Doctorate in Sciences (2015) from the Institute of Physics "Gleb Wataghin" of UNICAMP. Was a post-doc at the "Instituto de Astronomia, Geofísica e Ciências Atmosféricas" of Universidade de São Paulo (2015-2018) and at UNICAMP (2018-2019). Currently Adjunt Professor at Federal University of ABC. Has experience in Physics, focusing on Genelral Relativity and Gravitation and in Galactic Dynamics. (Source: Lattes Curriculum)
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The modeling of orbits in general relativity is an essential field of study in astrophysics.In particular, the study of galactic dynamics is based on analyzing the orbits in metrics with axial symmetry. Several works involving orbital dynamics of stars in the Milky Way model the Galactic diskby Miyamoto-Nagai's potential. Focusing on approaching the problem in general relativity, this pro…
This project aims to study the Hamiltonian dynamics of test particles in Newtonian and relativistic discoidal systems, with emphasis mainly in the dynamics of stars in spiral galaxies (especially in the Milky Way). Our goal is to advance in the description of the Hamiltonian dynamics in these systems, focusing on two different aspects: (i) the regular motion around equilibrium points and …
Study of Newtonian and post-Newtonian self-gravitating structures with and whthout dark matter halos utilizing tools from dynamical systems. Study of chaos and stability in these models. Qualitative and computational analysis of the problem. Study of the distribution function for the disks and for dark matter.
(Only some records are available in English at this moment)
The general relativistic treatment of the radiation field of a spherically symmetric star introduces new features, which are absent in Newtonian gravity. One important result is the presence of the "Eddington Capture Sphere'', a radius for which the gravitational and radiation forces balance. This region is shown to be an attractor for the dynamics of test particles. We intent to deepen t…
| 5 / 4 | Completed scholarships in Brazil |
| 1 / 1 | Completed scholarships abroad |
| 6 / 5 | All Scholarships |
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