30.01, Alexander Stasik:
IceCube: A neutrino
telescope in the Antarctica
IceCube is a 1 km^3 neutrino telescope located at the geographical south
pole. It consists of 5160 photomultiplier deployed in the clear Antarctic
ice in a depth of 1450 m to 2450 m as well as an air shower array on the
surface. IceCube is designed to measure high energy neutrinos of all
flavours with a directional accuracy up to 1$^\circ$. This allows the study
of potential accelerators like active galactic nucleus, gamma ray bursts and
galactic objects like supernova remnants or pulsars as sources for high
energy neutrinos and cosmic rays. Furthermore IceCube allows indirect dark
matter search. The big number of atmospheric neutrinos created in air
showers allows a precise comparison with model predictions.
This talk will introduce the IceCube neutrino telescope and its detection
principle. Furthermore a mode of the detector, the optical follow-up, will
be presented. In that mode IceCube is used to trigger optical and
$\gamma$-ray telescopes in a transient object search.