Simulation of a hybrid optical-radio-acoustic neutrino detector at the South Pole

Details Simulation of a hybrid optical-radio-acoustic neutrino detector at the South Pole Simulation of a hybrid optical-radio-acoustic neutrino detector at the South Pole

2008-11-13

arxiv.org/abs/0811.2100v1

Nucl.Instrum.Meth.Suppl.A604:179-181,2009

Astronomy and Astrophysics

Astrophysics

4 pages, 5 figures,1 Table, to appear in the proceedings of the Acoustic and Radio EeV Neutrino detection Activities (ARENA) 2

Scientific paper

10.1016/j.nima.2009.03.047

With construction halfway complete, IceCube is already the most sensitive neutrino telescope ever built. A rearrangement of the final holes of IceCube with increased spacing has been discussed recently to optimize the high energy sensitivity of the detector. Extending this baseline with radio and acoustic instrumentation in the same holes could further improve the high energy response. The goal would be both to detect events and to act as a pathfinder for hybrid detection, towards a possible larger hybrid array. Simulation results for such an array are presented here.

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