CV Lattes
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Universidade de São Paulo (USP). Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Bachelor in Physics from the Instituto de Física - USP (2018). Currently, is a PhD student at the Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG - USP), where develops a project entitled "Cosmic Magnetism and Propagation of the Cosmic Ray in the Large-Scale Universe". Has carried out research in the field of Astronomy, with an emphasis on High Energy Astrophysics, working mainly on the following topics: AGN and SN Feedback, Electromagnetic Instabilities and Intergalactic Magnetic Fields. Worked as a volunteer physics teacher in the popular pre-university course Psico-USP, and is involved in several scientific dissemination projects such as the Astrominas Project, Monitored Visit-Astronomy Service for schools - and Astronomy for Teachers. She is also an organizer of the lecture series "Astronomia ao Meio Dia". (Source: Lattes Curriculum)
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This is a scholarship renewal solicitation to conclude the fifth year of the student's Ph.D. thesis who has a FAPESP scholarship (2019/04992-4) linked to the Thematic Project (2013/10559-5) coordinated by her advisor, which will be concluded in the coming July 31, 2023. During the first four years, most of the research of the initial Proposal has been carried out on studies of the origin …
In this PhD project, we intend to continue research studies developed in our group regarding the origin of cosmic magnetic fields in the diffuse Intergalactic Medium (IGM) and clusters of galaxies (de Gouveia Dal Pino 2011), as well as their connection with turbulence and Cosmic Ray (CR) propagation. Well tested three-dimensional numerical grid-based Godunov-MHD codes developed by the gro…
Primordial magnetic fields are amplified by turbulent dynamo effects, as well as by star-formation and stellar evolution processes in the InterStellar Medium of galaxies. At the same time, powerful galactic outflows are generated by energy feedback from various processes: stars, stellar evolution, and SuperNovae (SN) explosion, together with large-scale dynamical events, e.g. galaxy merge…
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