CV Lattes
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Universidade Estadual Paulista (UNESP). Campus de Guaratinguetá. Faculdade de Engenharia (FEG) (Institutional affiliation from the last research proposal) Birthplace: Brazil
PhD student of Physics at UNESP, Brazil. Master's degree in Physics at UNESP, Brazil. Graduated bachelor in Physics at UNESP, Brazil. Technician in Industrial Computation by the CTIG-UNESP, Brazil. Works in the area of Astronomy, specifically planetary formation. Has experience in programming. (Source: Lattes Curriculum)
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The formation of Uranus and Neptune is one of the great challenges of the planetary formation models. Most models assume that supermassive planetary embryos exist beyond Saturn's orbit, and by colliding with each other and/or accreting particles with sizes of cm and mm (known as pebbles) give rise to the Uranus and Neptune cores shortly before the solar nebula dissipation. The models fail…
For simplicity, most planet formation models assume that collisions during the intermediate and final phases of planetary formation are constructive. This type of approach has been used both in solar system and exoplanet formation models. The objective of this master's thesis project is to study the impact of a more realistic collision treatment in numerical simulations modeling the forma…
For simplicity, most planet formation models assume that collisions during the intermediate and final phases of planetary formation are constructive. This type of approach has been used both in solar system and exoplanet formation models. The objective of this master's thesis project is to study the impact of a more realistic collision treatment in numerical simulations modeling the forma…
The main goal of this project is to contribute to the formation of an undergraduate student in the context of presenting to the student an updated view on planetary formation theories. The number of exoplanets confirmed today is larger than 2000. These new exoplanetary systems are providing a variety of new constraints to theoretical models which 10 or 20 years ago were only offered by ou…
The magma oceans on the surface of planets are an important issue in understanding the evolution of atmospheric composition and the mantle-to-core mass ratio of planets. The molten magma is constantly vaporized releasing heavy chemical species from the mantle into the atmosphere. The atmospheric escape of these heavy materials from the magma is favored when in contact with a hydrogen atmo…
| 1 / 1 | Ongoing scholarships in Brazil |
| 3 / 3 | Completed scholarships in Brazil |
| 1 / 1 | Completed scholarships abroad |
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