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...'''Glashow resonance''' is the resonant formation of the [[W boson]] in [[neutrino|antineutrino]]-electron collisions: {{SubatomicParticle|Electron antineutri ...te=2020-02-18 |title=$W$-boson and trident production in TeV--PeV neutrino observatories |journal=Physical Review D |volume=101 |issue=3 |pages=036010 |doi=10.1103/ ...

...fold coincidence technique.<ref>Cowan, C. L. et al. "Detection of the Free Neutrino: a Confirmation." ''Science'', vol. 124, no. 3212, 20 Jul. 1956, p. 448, DO === Conan and Reines' neutrino experiment === ...

...first15=T. |title=STEREO neutrino spectrum of 235U fission rejects sterile neutrino hypothesis |url=https://www.nature.com/articles/s41586-022-05568-2 |journal ...blue and red show the case including the oscillation into a light sterile neutrino]] ...

...al|last=Mondal|first=Naba K.|date=January 2004|title=Status of India-based Neutrino Observatory (INO)|url=http://www.imsc.res.in/~ino/OpenReports/Insa/naba.pdf .../2015/Friday/Zelimir%20Djurcic%20-%20JUNO.pdf |title=Status of India-Based Neutrino Observatory (INO) |first=B S |last=Acharya |location=Madison, Wisconsin |da ...

...used.}} are considered the strongest and most frequent source of [[cosmic neutrino]]s in the MeV energy range. ...]] phenomena.<ref name=":15" /> Further, coincident detection of supernova neutrino in different experiments would provide an early alarm to [[astronomer]]s ab ...

{{Short description|Neutrino physics experiment in Italy}} | title = Borexino neutrino observatory ...

...sars]] in [[binary star]] systems. The [[waveform]], detected by both LIGO observatories,<ref name="BBC_11Feb16" /> matched the predictions of [[general relativity] LIGO operates two [[Gravitational-wave observatory|gravitational-wave observatories]] in unison, located {{convert|3002|km|mi|abbr=on}} apart: the LIGO Livings ...

...ch as the [[Super-Kamiokande]], the [[Sudbury Neutrino Observatory|Sudbury Neutrino Observatory (SNO)]] and [[IceCube]]. Other projects operated in the past ap Astrophysics observatories using the Cherenkov technique to measure air showers are key to determining ...

...S. |last2=de Holanda |first2=P. C. |last3=Saa |first3=A. |date=2021 |title=Neutrino primordial Planckian black holes |journal=Physics Letters |volume=B822 |pag '''Fast Radio Bursts observatories''' ...

...ino decoupling|neutrinos decouple]]; these [[neutrino]]s form the [[cosmic neutrino background]] (CνB). If [[primordial black hole]]s exist, they are also form | [[Neutrino decoupling]] ...

...universe's most elusive components: [[dark matter]], [[dark energy]] and [[neutrino]]s.<ref>{{cite web ...nt.<ref>{{cite journal |last1=Campbell |first1=W. W. |title=Reports of the Observatories: Lick Observatory |journal=Publications of the Astronomical Society of the ...

...-messenger detection]] (electromagnetic and gravitational radiation, and [[neutrino]]s) would help to better understand the supernova process and the formation ...oordinates Network|GCN]], which also centralizes alerts from gamma-ray and neutrino telescopes, as well as [[SciMMA]].<ref>{{Cite web |title=GCN – General Coor ...

...veloped a method for measurement of [[stellar rotation]], directed several observatories in the US ...kheyev]]''', co-discoverer of [[Mikheyev–Smirnov–Wolfenstein effect]] of [[neutrino oscillations]] ...