EPJ Web of Conferences
Volume 121, 2016Roma International Conference on Astroparticle Physics 2014 (RICAP-14)
|Number of page(s)||8|
|Section||High Energy Neutrinos|
|Published online||06 July 2016|
Neutrinos from Gamma Ray Bursts in the IceCube and ARA Era
1 ORT Braude College, Carmiel, Israel
2 INAF-OAR Monteporzio Catone, Italy
a e-mail: firstname.lastname@example.org
Published online: 6 July 2016
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.
© The Authors, published by EDP Sciences
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
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