Speaker
Prof.
Tomasz Bulik
(University of Warsaw)
Description
Gravitational wave sources detected by LIGO Virgo and Kagra are primarily BBH but also there arre several detections of events that include neutron stars. Theses objects are primary candidates for multimessenger sources as there is plenty of matter available. I will review the current status of the observations, and the constraints on their rate density. The turbulent environment around such mergers is very likely to lead to particle acceleration. I will discuss the chances of detecting such particles - cosmic rays - in the next year's and with the next generation instruments.
Primary author
Prof.
Tomasz Bulik
(University of Warsaw)
