CV Lattes
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Universidade do Vale do Paraíba (UNIVAP). Instituto de Pesquisa e Desenvolvimento (IP&D) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Degree in Physics from Física pelo Instituto Federal de Educação, Ciência e Tecnologia do Ceará (IF-CE, 2010). MSc from Universidade Federal de Itajubá (UNIFEI - 2012) in astrophisics of dense molecular clouds. PhD from Universidade do Vale do Paraíba (UNIVAP/FAPESP - 2015) in computational simulation of star-forming regions and spectroscopic analysis of astrophysical ices processed in laboratory. Post-doc at the same institution working on the same research area. Post-doc at University of St. Andrews, Escócia (2017-2018) working on computational simulation of irradiated ices. Currently works as post-doc at the University of Copenhagen on the identification of complex organic molecules in star-forming regions via computational simulation and interferometry. The reseach interest regards to observation of complex molecules in early and late phases of stellar formation, laboratory experiments of astrophysical ices and IR and sub-mm observations. Expertise in using computational codes such as NKABS, RADMC-3D, KROME, ProDiMo, and MC-Max 3D. (Source: Lattes Curriculum)
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It has been shown through observations in the infrared from ISO (Infrared Space Observatory) and SST (Spitzer Space Telescope), the existence of astrophysical ices toward protostars. Among them, there are H2O, CO, CO2, NH3, CH3OH, CH4, HCOOH, H2CO, CH3CHO. In the same time of observations, several papers were published, showing the formation of complex molecules from simple one, through e…
The aims of the project is to study the radiation-matter interaction inside dense molecular clouds using optical properties of interstellar grains determined from experimental data at the infrared wavelength region and computational model.
Protoplanetary disks host simple and complex molecules in the gas phase and in the condensed state, from which new planets are formed. The formation and survival of these molecules is affected by the temperature and the UV and X-ray radiation field in the disk. To address these questions, laboratory and theoretical efforts are essential to determine where molecular species are destroyed o…
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