Radiative magnetic reconnection in black hole and neutron star magnetospheres.
ORAL
Abstract
In this talk I will review recent progress in modeling magnetic reconnection in the regime of dynamically important radiative losses. I will highlight applications to modeling multi-wavelength non-thrermal emission from neutron stars and flares from accreting supermassive black holes.
*This research is supported by NSF-DOE partnership (grant no. PHY-2010145) and NASA (grant no. 80NSSC22K1054).
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Presenters
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Alexander A Philippov
- University of Maryland, College Park
- University of Maryland