CORDIS Project
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This project investigates the mechanisms behind coherent radio emissions from neutron stars, focusing on the role of plasma instabilities and kinetic Alfvén waves. By utilizing advanced simulations, it aims to predict the properties of these emissions, contributing to our understanding of pulsars and fast radio bursts.
Magnetospheres of neutron stars (NSs) represent unique plasma-physics labs of extreme environments characterized by ultra-high magnetic field strengths, relativistic processes, and the presence of quantum electrodynamic effects – parameters far unreachable on the Earth.
Detailed information on these processes comes to us via coherent radio emissions of pulsars and possibly fast radio bursts (FRBs), being observed by fast-developing sophisticated instruments of radio astronomy like FAST, CHIME, A…
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