Radiation of Extreme Plasmas near the Neutron Stars and Black holes
APA
Philippov, A. (2025). Radiation of Extreme Plasmas near the Neutron Stars and Black holes. Perimeter Institute. https://pirsa.org/25030178
MLA
Philippov, Alexander. Radiation of Extreme Plasmas near the Neutron Stars and Black holes. Perimeter Institute, Mar. 26, 2025, https://pirsa.org/25030178
BibTex
@misc{ pirsa_PIRSA:25030178, doi = {10.48660/25030178}, url = {https://pirsa.org/25030178}, author = {Philippov, Alexander}, keywords = {Other}, language = {en}, title = {Radiation of Extreme Plasmas near the Neutron Stars and Black holes}, publisher = {Perimeter Institute}, year = {2025}, month = {mar}, note = {PIRSA:25030178 see, \url{https://pirsa.org}} }
Alexander Philippov University of Maryland, College Park
Abstract
Astrophysical compact objects, neutron stars, and black holes are powerful sources of non-thermal electromagnetic emission spanning many orders of magnitude in photon energy, from radio waves to multi-TeV gamma rays. Despite multiple groundbreaking observational discoveries done in recent years, our understanding of the dynamics of relativistic plasmas that produce these emission signatures remains limited. In this talk, I will describe a few successful examples of modeling the observed light coming from these remarkable astrophysical laboratories using various numerical approaches. I will focus on advances in understanding coherent radio emission of rotating neutron stars, pulsars, and multi-wavelength flares from accreting black holes.