- Astrophysical neutrinos are high-energy neutrinos that originate from the farthest reaches beyond our galaxy.
- As they travel massive distances undisturbed, they can help us understand about evolution of universe.
- About Neutrinos
- Neutrinos are subatomic particles that have no electrical charge and very small mass, which might even be zero.
- They are the most abundant particles in the universe and they have very little interaction with matter.
- Neutrinos travel close to speed of light and are incredibly difficult to detect, hence called “ghost particles”.
- They are produced through many natural processes such as Sun’s nuclear reactions, particle decays in Earth etc., particle accelerators and nuclear power plants.
- Neutrinos come in three different flavors: electron, muon and tau.
- About IceCube, the South Pole Neutrino Observatory
- It is a cubic-kilometer neutrino particle detector, located near the Amundsen-Scott South Pole Station.
- IceCube is the first gigaton neutrino detector ever built and was primarily designed to observe neutrinos from the most violent astrophysical sources.
- It uses “strings” (cables) of digital optical modules (DOMs) to detect neutrinos.
- In 2013, IceCube presented its first evidence of high-energy astrophysical neutrinos originating from cosmic accelerators.
India-based Neutrino Observatory (INO) Project
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