Supernova neutrinos are weakly interactive elementary particles produced during a core-collapse supernova explosion. A massive star collapses at the end...

small mass of the neutrino, and neutrinos do not participate in the electromagnetic interaction or the strong interaction. Thus, neutrinos typically pass...

The diffuse supernova neutrino background (DSNB) is a theoretical population of neutrinos (and anti-neutrinos) cumulatively originating from all core-collapse...

A neutrino detector is a physics apparatus which is designed to study neutrinos. Because neutrinos only weakly interact with other particles of matter...

light-years) from Earth and was the closest observed supernova since Kepler's Supernova in 1604. Light and neutrinos from the explosion reached Earth on February...

doi:10.1063/1.1291879. S2CID 5803494. Beacom, J. F. (1999). "Supernova neutrinos and the neutrino masses". Revista Mexicana de Fisica. 45 (2): 36. arXiv:hep-ph/9901300...

sources of neutrinos- such as neutrinos released by supernovae- have been detected. Several neutrino experiments have formed the Supernova Early Warning...

away". This is accomplished by a further release of neutrinos. These 'thermal' neutrinos form as neutrino-antineutrino pairs of all flavors, and total several...

and neutrinos: p + e− → n + νe. It is expected that the neutrinos are emitted well before the light from the supernova peaks, so in principle neutrino detectors...

A supernova is an event in which a star destroys itself in an explosion which can briefly become as luminous as an entire galaxy. This list of supernovae...

contemporary neutrino observatories. The supernova 1987A indicated that neutrinos might have mass because of the difference in time of arrival of the neutrinos detected...

energy spectrum of events. Neutrino oscillations Chela-Flores 2011, p. 305. When neutrinos go through the MSW resonance the neutrinos have the maximal probability...

now-resolved solar neutrino problem. Much is now known about solar neutrinos, but research in this field is ongoing. The timeline of solar neutrinos and their...

neutrino background (CNB or CνB) is the universe's background particle radiation composed of neutrinos. They are sometimes known as relic neutrinos....

Neutrino experiments are scientific studies investigating the properties of neutrinos, which are subatomic particles that are very difficult to detect...

solar neutrinos, geoneutrinos from radioactive decays in the Earth, and reactor neutrinos. It could also observe supernovae neutrinos if a supernova occurs...

the Supernova Early Warning System (SNEWS). A signature of sterile neutrinos would be a distortion of the energy spectrum of atmospheric neutrinos around...

observe solar neutrinos. As a result, the detector (KamiokaNDE-II) had become sensitive enough to detect ten neutrinos from SN 1987A, a supernova which was...

cosmic rays, and the 1987 detection of neutrinos emitted from Supernova SN1987A, which inaugurated the field of neutrino astronomy. Frederick Reines was born...

They found agreement of neutrino speed with the speed of light. The experiment created a form of neutrinos, muon neutrinos, at CERN's older SPS accelerator...

neutrino luminosities, and the additional neutrinos emitted help re-energize the shock wave. These changes remove some, but not all, of the supernova...

Supernova nucleosynthesis is the nucleosynthesis of chemical elements in supernova explosions. In sufficiently massive stars, the nucleosynthesis by fusion...

neutrino oscillations must be observed in matter. With HK beam neutrinos (295 km, 600 MeV), the matter effect is small. In addition to beam neutrinos...

helium-3 neutron detectors from the Sudbury Neutrino Observatory. The idea of using lead to detect supernova neutrinos was originally proposed in 1996 by Cliff...

of solar neutrinos reaching the Earth were taken in the 1960s, and all experiments prior to SNO observed a third to a half fewer neutrinos than were...

in solar flares. 1987: Supernova SN 1987A emitted neutrinos that were detected at the Kamiokande-II, IMB and Baksan neutrino observatories, a couple...

A Type Ia supernova (read: "type one-A") is a type of supernova that occurs in binary systems (two stars orbiting one another) in which one of the stars...

Cowan–Reines neutrino experiment was conducted by physicists Clyde Cowan and Frederick Reines in 1956. The experiment confirmed the existence of neutrinos. Neutrinos...

A near-Earth supernova is an explosion resulting from the death of a star that occurs close enough to the Earth (roughly less than 10 to 300 parsecs [30...

available in a particular flavour of neutrinos but also through other general-relativistic effects on neutrinos. Some evidence gained from analysis of...