Overview
Explore the cutting-edge developments in high-energy neutrino astronomy through this keynote plenary session presented by Marcos Santander at the APS April Meeting 2019. Delve into the fascinating world of cosmic messengers, focusing on neutrinos and their ability to traverse vast cosmic distances unimpeded. Examine the detection principles of gigaton-scale detectors and learn about the current generation of neutrino observatories. Discover the significance of the 2013 IceCube discovery of an astrophysical neutrino flux and the 2017 identification of a blazar as a potential neutrino source. Investigate various neutrino sources, including the galactic plane and gamma-ray bursts, and explore future prospects in neutrino astronomy. Gain insights into ongoing and planned neutrino detection efforts at Lake Baikal, the Mediterranean Sea, and the South Pole, concluding with an overview of the neutrino flux and its implications for our understanding of the universe.
Syllabus
Introduction
Cosmic messengers
Neutrino fluxes
Cosmic rays
Gigaton scale detectors
Detection principle
Current generation
Neutrino astronomy
Astrophysical neutrinos
Galactic neutrinos
Physical neutrinos
Neutrino sources
Galactic plane
Gammaray bursts
IceCube neutrino event
Blazer neutrino event
Astrophysical neutrino detection
Interest in time
Lake Baikal
Mediterranean Sea
South Pole
Neutrino flux
Conclusion
Questions
Taught by
APS Physics