High Energy and Plasma Astrophysics Group (GAPAE)

Most of the visible matter in the Universe is in a plasma state, or more specifically is composed of ionized or partially ionized gas permeated by magnetic fields.

My group develops several correlated studies employing theoretical and numerical magneto-hydrodynamics (MHD) description to investigate astrophysical plasmas and high energy phenomena. Our multi-dimensional MHD numerical simulations employ high performance computing (HPC) with sophisticated codes on studies of:

My group is also involved in the Cherenkov Telescope Array (CTA), an international collaboration aiming at the construction of a new generation of gamma ray telescopes—an array of 120 Cherenkov telescopes.

My group has obtained funding from FAPESP for the construction of the ASTRI Mini-Array of 9 Cherenkov telescopes, the CTA precursor.

Ongoing Supervisions

Former Graduate Students – PhD

Former Graduate Students – Master

Former Postdoctoral Fellows