CORDIS Project
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This project investigates the dynamics of magnetic reconnection in high-energy astrophysical environments, such as those surrounding neutron stars and black holes. By utilizing advanced simulation techniques, it aims to understand how this process accelerates particles and produces radiation, enhancing our knowledge of…
Astrophysical compact objects like neutron stars and black holes are surrounded by a hot gas of charged particle known as plasma.
In these environments, we observe powerful phenomena, including pulsar wind nebulae, jets, and gamma-ray bursts.
The mechanisms behind particle acceleration and high-energy emissions, particularly magnetic reconnection, are not fully understood.
Magnetic reconnection, where magnetic field lines break and reconnect, is believed to drive particle acceleration up to ultr…
KATHOLIEKE UNIVERSITEIT LEUVEN
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