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SUMMARY:Cosmic neutrino searches with the KM3NeT neutrino detector: a mult
 i-messenger approach
DTSTART;VALUE=DATE-TIME:20251120T081500Z
DTEND;VALUE=DATE-TIME:20251120T083000Z
DTSTAMP;VALUE=DATE-TIME:20260420T202024Z
UID:indico-contribution-28890@indico.ific.uv.es
DESCRIPTION:Speakers: Juan Palacios González (IFIC)\nMulti-messenger astr
 onomy is an emerging field that aims to combine the information carried by
  different cosmic messengers (cosmic rays\, photons\, neutrinos\, and grav
 itational waves) originating at a common source. Neutrinos\, being stable 
 and neutral particles\, are especially valuable as they can escape dense e
 nvironments. Furthermore\, they are not absorbed during propagation to Ear
 th and constitute an unambiguous signature for hadronic processes at the s
 ource.\nKM3NeT is a deep-sea infrastructure currently under construction a
 t the bottom of the Mediterranean Sea\, hosting a 3-dimensional array of l
 ight sensors designed to detect the Cherenkov light induced by neutrino in
 teractions. Two separate arrays are already operational using partial conf
 igurations: ORCA\, optimised for the GeV-TeV energy range\, and ARCA\, opt
 imised for the TeV-PeV energy range. In this talk\, the latest results of 
 the real-time follow-up searches for neutrino counterparts in coincidence 
 with external triggers are presented\, with special emphasis on the follow
 -up to gravitational wave events. In addition to these real-time studies\,
  a stacking search for cosmic neutrinos coming from gamma-ray bursts is al
 so presented\, conducted using data from the period when ARCA was operatio
 nal with 21 detection lines.\n\nhttps://indico.ific.uv.es/event/8035/contr
 ibutions/28890/
LOCATION:
URL:https://indico.ific.uv.es/event/8035/contributions/28890/
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