Modeling Magnetic Dissipation in Magnetar Magnetospheres
Kavli Institute for Theoretical Physics via YouTube
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Explore the complex physics of magnetic dissipation in magnetar magnetospheres through this 18-minute conference talk by Michael Grehan from CITA. Delve into the extreme plasma processes occurring around these exotic neutron stars, where magnetic fields reach extraordinary strengths and create unique astrophysical phenomena. Learn about the theoretical modeling approaches used to understand how magnetic energy is dissipated in these extreme environments, where relativistic, radiative, and quantum electrodynamic effects become critically important. Examine the challenges of modeling nonlinear plasma processes like magnetic reconnection under the extreme conditions found in magnetar magnetospheres, and discover how these processes contribute to the spectacular observational phenomena associated with these objects. Gain insights into the intersection of plasma physics, high-energy astrophysics, and computational modeling as applied to understanding some of the most magnetically extreme objects in the universe.
Syllabus
Modeling Magnetic Dissipation in Magnetar Magnetospheres | Michael Grehan (CITA)
Taught by
Kavli Institute for Theoretical Physics