Speaker
Ms
Oleksandra Ostapenko
(Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)
Description
Gamma-ray bursts are thought to be accelerators of cosmic rays and a source of high-energy astrophysical neutrinos. Nevertheless, none of previous GRBs researches have shown a correlation between particular events and high-energy neutrinos. In the light of the first detection of TeV gamma-ray emission from GRB190114C, our goal is to explore the possibility of detecting the neutrino fluxes coming from similar events based on the observed gamma-ray fluxes.
We present a calculation of neutrino fluxes from GRB190114C for different neutrino telescopes, and we calculate the total integrated emission expected from similar sources.
Author
Ms
Oleksandra Ostapenko
(Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)
Co-authors
Juan Pablo Yanez Garza
(Faculty of Science, University of Alberta)
Nahee Park
(Department of Physics, Queen's University)
