IceCube Neutrino Observatory

The IceCube Neutrino Observatory is a neutrino telescope constructed at the Amundsen–Scott South Pole Station in Antarctica. Its thousands of sensors are distributed over a cubic kilometre of volume under the Antarctic ice. Similar to its predecessor, the Antarctic Muon And Neutrino Detector Array, IceCube consists of spherical optical sensors called Digital Optical Modules, each with a photomultiplier tube and a single board data acquisition computer which sends digital data to the counting house on the surface above the array. IceCube was completed on 18 December 2010.

IceCube is a particle detector at the South Pole that records the interactions of a nearly massless  subatomic particle called the neutrino. IceCube searches for neutrinos from the most violent astrophysical sources: events like exploding stars, gamma-ray bursts, and cataclysmic phenomena involving black holes and neutron stars.

The IceCube telescope is a powerful tool to search for dark matter and could reveal the physical processes associated with the enigmatic origin of the highest energy particles in nature. In addition, exploring the background of neutrinos produced in  the atmosphere, IceCube studies the neutrinos themselves; their energies far exceed those produced by accelerator beams. IceCube is the world’s largest neutrino detector, encompassing a cubic kilometre of ice.

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