Overview
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Explore global kinetic models of spider pulsars in this 31-minute conference talk delivered at the Kavli Institute for Theoretical Physics. Delve into the complex physics governing these exotic binary systems where a pulsar's energetic wind interacts with a companion star, creating fascinating astrophysical phenomena. Learn how advanced kinetic modeling approaches help scientists understand the relativistic plasma processes occurring in these extreme environments, where magnetic reconnection, particle acceleration, and radiation mechanisms operate under conditions far beyond terrestrial laboratory capabilities. Discover how these models contribute to our broader understanding of neutron star physics and the behavior of relativistic plasmas in astrophysical contexts. Gain insights into the computational challenges and theoretical frameworks required to simulate these systems, including the treatment of relativistic effects, magnetic field dynamics, and particle interactions that characterize spider pulsar systems.
Syllabus
Global kinetic models of spider pulsars | Lorenzo Sironi (Columbia)
Taught by
Kavli Institute for Theoretical Physics