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In this review I discuss the ultra-high energy neutrinos (UHEN) originatedfrom Cosmic-Rays propogation (GZK neutrinos) and from Gamma Ray Bursts (GRBs),and discuss their detectability in kilometers scale detectors like ARA andIceCube.  While GZK neutrinos are expected from cosmic ray interactions on the CMB, theGRB neutrinos depend on the physics inside the sources. GRBs are predicted toemit UHEN in the prompt and in the later 'after-glow' phase.  I discuss the constraints on the hadronic component of GRBs derived from thesearch of four years of IceCube data for a prompt neutrino fux from gamma-raybursts (GRBs) and more in general I present the results of the search forhigh-energy neutrinos interacting within the IceCube detector between 2010 and2013.

Neutrinos from Gamma Ray Bursts in the IceCube and ARA Era