![neutrino telescopes neutrino telescopes](https://cerncourier.com/wp-content/uploads/2012/07/CCmed1_06_12.jpg)
![neutrino telescopes neutrino telescopes](https://ibgnews.com/wp-content/uploads/2017/03/India-Space-Update-Indian-Neutrino-Observatory.jpg)
The ORCA telescope is the instrument for KM3NeT scientists studying neutrino properties exploiting neutrinos generated in the Earth's atmosphere.Īrrays of thousands of optical sensors will detect the faint light in the deep sea fromĬharged particles originating from collisions of the neutrinos and the Earth.
![neutrino telescopes neutrino telescopes](https://news-cdn.softpedia.com/images/news2/NSF-Selects-Neutrino-Telescope-Operators-2.jpg)
The cosmic rays produce many muons which penetrate deeply into the earth, in even the deepest mines, but of course with ever decreasing numbers with. With the ARCA telescope, KM3NeT scientists will search for neutrinos from distant astrophysical sources such as supernovae, gamma ray bursters or colliding stars. Neutrino detectors must be generally placed deep underground or water to escape the backgrounds caused by the inescapable rain of cosmic rays upon the atmosphere. Located in the deepest seas of the Mediterranean, KM3NeT will open a new window on our Universe, but also contribute to the research of the properties of the elusive neutrino particles. Once completed, the telescopes will have detector volumes between megaton and several cubic kilometres of clear sea water. High-energy phenomena such as supernovas and X-ray double stars may emit a flood of neutrinos. AMANDA and its extensions should have the best discovery potential once WIMP masses exceed 200 GeV 10. This is often illustrated by their capability to detect the annihilation into high-energy neutrinos of neutralinos, the lightest supersymmetric particle which may constitute the cold dark matter. Neutrino detectors must be generally placed deep underground or water to escape the backgrounds caused by the inescapable rain of cosmic rays upon the atmosphere. KM3NeT is a research infrastructure housing the next generation neutrino telescopes. Neutrino telescopes can do particle physics. Thus a detector can effectively collect the results of neutrino interactions from a target volume much greater than the detector volume itself.