NBIA Astroparticle Seminar: Lisa Schumacher

The discovery of high-energy astrophysical neutrinos by IceCube has undoubtedly started the field of high-energy neutrino astronomy. However, the current observation rate of astrophysical neutrinos in the TeV-PeV energy range remains low, leaving open questions about the sources of high-energy neutrinos in our Galaxy and beyond. This observation rate will drastically improve as additional neutrino telescopes in the Northern Hemisphere come online in the next years. In this talk, I will present the status and prospects of the Pacific Ocean Neutrino Experiment (P-ONE). Located off the coast of Vancouver Island in the Pacific Ocean, P-ONE will complement the field of view of KM3NeT in the Mediterranean Sea and IceCube at the South Pole. I will introduce the concept of the Planetary Neutrino Monitoring network (PLEnuM) to show that the strength of the new neutrino telescopes will lie in their complementarity and their combined exposure.