Contact: lcombi[AT]perimeterinstitute.caLocation: Waterloo, Canada
In the vicinity of neutron stars and black holes, where spacetime is strongly curved, magnetic fields can power many of the violent phenomena that we observe across the entire electromagnetic spectrum, from accretion and jet launching, to magnetar flares and pulsar emission. In the last decades, our theoretical understanding of the role of magnetic fields in these extreme environments has greatly improved through numerical simulations of magnetohydrodynamical fluids and charged kinetic particles; however, many open and important questions remain. Our observational capabilities and computational resources will keep growing dramatically in the next few years, allowing us to explore high-energy astrophysics in unprecedented regimes. Improving our knowledge of how magnetic fields, matter, and gravity interact with each other is a crucial piece in the new era of multimessenger astrophysics.
This workshop will gather experts from a wide range of disciplines within physics and astrophysics to present state-of-the-art advances in theoretical models of magnetic fields and high-energy plasma in different contexts, from neutron star mergers to supermassive black holes, and from micro scales to macro scales.
Scientific Organizers:
Luciano Combi (Perimeter Institute and U of Guelph)
Sean Ressler (CITA)
Bart Ripperda (CITA)
Luis Lehner (Perimeter Institute)
Will East (Perimeter Institute)
Gibwa Musoke (CITA)
Chris Thompson (CITA)