Speaker
Dr
Tetyana Pitik
(University of Berkeley)
Description
A growing number of luminous optical transients from stellar explosions are believed to be powered by the interaction between ejected stellar material and a dense circumstellar medium. This interaction drives shock waves that can accelerate particles to multi-PeV energies, producing radiation across a broad range of wavelengths. In this talk, I will explore the connection between multi-wavelength electromagnetic signatures and high-energy neutrino production, and discuss the prospects for joint detection across current and future observatories.
Primary author
Dr
Tetyana Pitik
(University of Berkeley)
