The Prediction and Detection of UHE Neutrino Bursts
Mou Roy (LBNL), H.J. Crawford (LBNL), Athena Trattner (LBNL)

TL;DR
This paper proposes a cost-effective km^2 detector in deep water to observe ultra-high-energy neutrino bursts associated with gamma ray bursts, enabling tests of fundamental physics principles.
Contribution
It introduces an efficient design for a large-area neutrino detector in deep water, optimized for detecting UHE neutrino bursts coincident with GRBs.
Findings
Estimated detection of ~20 neutrino events in one year
Detector construction cost under $3 million
Potential to test relativity principles through coincident observations
Abstract
In this paper we look at \sim 10^14 eV neutrino bursts which are predicted to be observed in correlation with gamma ray bursts (GRBs). We describe an efficient way of constructing a km^2 effective area detector for these neutrino bursts. The proposed detector will cost <$3M and will operate in the 4-km deep water off St.Croix for at least one year, sufficient time to collect the expected \sim 20 events in coincidence with satellite measured GRBs provided the fireball model is correct. Coincident gamma ray and neutrino bursts can be used to test the limits of the relativity principles.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
