BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:High-energy neutrino astronomy
DTSTART;VALUE=DATE-TIME:20191213T153000Z
DTEND;VALUE=DATE-TIME:20191213T170000Z
DTSTAMP;VALUE=DATE-TIME:20260610T123634Z
UID:indico-event-3932@indico.ific.uv.es
DESCRIPTION:More than 100 years after the discovery of cosmic rays\, their
  origin and acceleration mechanisms are a yet unresolved puzzle that neutr
 inos have the chance to solve. Being chargeless and weakly-interacting\, n
 eutrinos can travel long distances without being deflected by cosmic magne
 tic fields and can escape dense celestial environments\, allowing for prec
 ise pointing to their production sites. Their detection will make it possi
 ble to unequivocally identify the sources of cosmic rays. While being the 
 perfect cosmic messengers\, neutrinos are extremely difficult to detect\, 
 requiring the construction of huge telescopes in unfriendly environments. 
 The detection principle of high-energy neutrinos\, the analysis method use
 d to identify cosmic neutrino sources\, and the latest results in the fiel
 d of high-energy neutrino astronomy are discussed in this talk.\n\nhttps:/
 /indico.ific.uv.es/event/3932/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/3932/
END:VEVENT
END:VCALENDAR