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The '''Glashow resonance''', put forward by [[Sheldon Lee Glashow|Sheldon L. Glashow]] in 1959, is the resonant formation of the [[W boson]] in antineutrino-electron collisions: {{SubatomicParticle|Electron antineutrino}} + {{SubatomicParticle|Electron-}} → {{SubatomicParticle|W boson-}}.<ref>{{cite journal | last=Glashow | first=Sheldon L. | title=Resonant Scattering of Antineutrinos | journal=Physical Review | publisher=American Physical Society (APS) | volume=118 | issue=1 | date=1960-04-01 | issn=0031-899X | doi=10.1103/physrev.118.316 | pages=316–317}}</ref> The threshold antineutrino energy for this process (for the electron at rest in the laboratory frame) is 6.3 [[electronvolt|PeV]]. This process is considered for the detection and studies of high-energy cosmic neutrinos at the [[IceCube Neutrino Observatory|IceCube experiment]], at the [[ANTARES (telescope)|ANTARES neutrino telescope]], and at the [[KM3NeT| KM3NeT neutrino telescope]]. |
The '''Glashow resonance''', put forward by [[Sheldon Lee Glashow|Sheldon L. Glashow]] in 1959, is the resonant formation of the [[W boson]] in antineutrino-electron collisions: {{SubatomicParticle|Electron antineutrino}} + {{SubatomicParticle|Electron-}} → {{SubatomicParticle|W boson-}}.<ref>{{cite journal | last=Glashow | first=Sheldon L. | title=Resonant Scattering of Antineutrinos | journal=Physical Review | publisher=American Physical Society (APS) | volume=118 | issue=1 | date=1960-04-01 | issn=0031-899X | doi=10.1103/physrev.118.316 | pages=316–317}}</ref> The threshold antineutrino energy for this process (for the electron at rest in the laboratory frame) is 6.3 [[electronvolt|PeV]]. This process is considered for the detection and studies of high-energy cosmic neutrinos at the [[IceCube Neutrino Observatory|IceCube experiment]], at the [[ANTARES (telescope)|ANTARES neutrino telescope]], and at the [[KM3NeT| KM3NeT neutrino telescope]]. |
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Revision as of 17:35, 31 May 2020
 | This article needs additional citations for verification. (February 2018) |
The Glashow resonance, put forward by Sheldon L. Glashow in 1959, is the resonant formation of the W boson in antineutrino-electron collisions:
ν
e +
e−
→
W−
.[1] The threshold antineutrino energy for this process (for the electron at rest in the laboratory frame) is 6.3 PeV. This process is considered for the detection and studies of high-energy cosmic neutrinos at the IceCube experiment, at the ANTARES neutrino telescope, and at the KM3NeT neutrino telescope.
References
- ^ Glashow, Sheldon L. (1960-04-01). "Resonant Scattering of Antineutrinos". Physical Review. 118 (1). American Physical Society (APS): 316–317. doi:10.1103/physrev.118.316. ISSN 0031-899X.
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