who initiated the studies on this?
Neutrinos were first recorded in 1956 by Clyde Cowan and Frederick Reines in an experiment employing a nearby nuclear reactor as a neutrino source.
Neutrino astronomy
Neutrinos were first recorded in 1956 by Clyde Cowan and Frederick Reines in an experiment employing a nearby nuclear reactor as a neutrino source.
what area of science did the muslim world excel in Astronomy, mathematics, and medicine. what does the first one refer to? The natural science that studies celestial objects and phenomena. what is it further classified into? Observational, radio, Infrared, Optical , Ultraviolet, X-ray and Gamma-ray astronomy. what are the leading types of the second area? UNANSWERABLE are there any foundations associated with it? Yes, in nutrino astronomy, GALLEX or Gallium Experiment was a radiochemical neutrino detection experiment that ran between 1991 and 1997 at the Laboratori Nazionali del Gran Sasso (LNGS). what does the the kind of astronomy mean? It  is the branch of astronomy that observes astronomical objects with neutrino detectors in special observatories. what are it's applications? It is used for observing the cores of stars. what methods of detection does it include? The detector must be at least 1 km deep to suppress downward traveling muons, and are subject to an irreducible background of extraterrestric neutrinos interacting in the Earth's atmosphere. what sort of detector is used for this? Detectors that consist of an array of photomultiplier tubes (PMTs) housed in transparent pressure spheres which are suspended in a large volume of water or ice.
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Neutrino astronomy [SEP] History
Neutrinos were first recorded in 1956 by Clyde Cowan and Frederick Reines in an experiment employing a nearby nuclear reactor as a neutrino source. Their discovery was acknowledged with a Nobel Prize for physics in 1995. This was followed by the first atmospheric neutrino detection in 1965 by two groups almost simultaneously. One was led by Frederick Reines who operated a liquid scintillator - the Case-Witwatersrand-Irvine or CWI detector - in the East Rand gold mine in South Africa at an 8.8 km water depth equivalent. The other was a Bombay-Osaka-Durham collaboration that operated in the Indian Kolar Gold Field mine at an equivalent water depth of 7.5 km.