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SUMMARY:Latest astrophysical and particle physics results and future prosp
 ects from IceCube
DTSTART;VALUE=DATE-TIME:20181023T070000Z
DTEND;VALUE=DATE-TIME:20181023T071500Z
DTSTAMP;VALUE=DATE-TIME:20260307T212345Z
UID:indico-contribution-1215@cern.ch
DESCRIPTION:Speakers: Thomas Stuttard (Niels Bohr Institute)\nThe IceCube 
 neutrino observatory uses a cubic km of deep South Pole ice instrumented w
 ith over 5000 optical sensors to detect Cherenkov light produced by astrop
 hysical and atmospheric neutrinos interacting in the ice. The detector pro
 bes neutrino energies from GeV to PeV\, propagation distances ranging from
  a few km to astrophysical scales\, and collects high statistics neutrino 
 samples due to its extremely large volume.\n\nIceCube has a broad physics 
 reach in both astrophysical and particle physics observations. Astrophysic
 al neutrinos are a crucial component of the nascent field of multimessenge
 r astronomy\, allowing observations of distant and extreme astrophysical p
 henomena. Additionally\, neutrinos of both astrophysical and atmospheric o
 rigin can be used to test our understanding of fundamental physics\, such 
 as neutrino oscillations and interactions with matter\, and to probe Beyon
 d Standard Model (BSM) theories.\n\nThis talk will present the latest resu
 lts from the IceCube collaboration and look ahead to future plans for next
  generation South Pole neutrino detection.\n\nhttps://indico.particle.meph
 i.ru/event/22/contributions/1215/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1215/
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