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Neutrinos from Gamma Ray Bursts in the IceCube and ARA Era

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

In this review I discuss the ultra-high energy neutrinos (UHEN) originated from Cosmic-Rays propogation (GZK neutrinos) and from Gamma Ray Bursts (GRBs), and discuss their detectability in kilometers scale detectors like ARA and IceCube. While GZK neutrinos are expected from cosmic ray interactions on the CMB, the GRB neutrinos depend on the physics inside the sources. GRBs are predicted to emit UHEN in the prompt and in the later "after-glow" phase. I discuss the constraints on the hadronic component of GRBs derived from the search of four years of IceCube data for a prompt neutrino fux from gamma-ray bursts (GRBs) and more in general I present the results of the search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2013.

Original languageEnglish GB
Title of host publicationRoma International Conference on Astroparticle Physics 2014, RICAP 2014
EditorsRosa Coniglione, Giulia De Bonis, Paolo Piattelli, Antonio Capone, Mario De Vincenzi, Carla Distefano, Aldo Morselli, Piera Sapienza
PublisherEDP Sciences
ISBN (Electronic)9782759890033
DOIs
StatePublished - 6 Jul 2016
Externally publishedYes
Event5th Roma International Conference on Astroparticle Physics, RICAP 2014 - Noto, Italy
Duration: 30 Sep 20143 Oct 2014

Publication series

NameEPJ Web of Conferences
Volume121

Conference

Conference5th Roma International Conference on Astroparticle Physics, RICAP 2014
Country/TerritoryItaly
CityNoto
Period30/09/143/10/14

ASJC Scopus subject areas

  • General Physics and Astronomy

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