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- {{Short description|Astronomical neutrinos produced during core-collapse supernova explosion}} ...igh Energy physics — PoS(ICHEP2020) |chapter=Core-Collapse Supernove Burst Neutrinos in DUNE |date=2021-04-15|language=en|publisher=SISSA Medialab|volume=390|pa ...37 KB (5,132 words) - 14:10, 4 October 2024
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- ....1016/0029-554X(77)90769-8|bibcode=1977NucIM.141..207C}}</ref> They detect neutrinos through the reaction:<ref>{{Cite journal|author=ICARUS-Collaboration|date=2 ...f [[modern physics]], neutrinos of astronomic or solar sources, and [[CERN Neutrinos to Gran Sasso]] (CNGS) [[Accelerator neutrino|beam]] produced 730 km a ...6 KB (871 words) - 00:30, 21 October 2024
- ...e=Collider neutrinos on the horizon|url=https://cerncourier.com/a/collider-neutrinos-on-the-horizon/|access-date=2021-08-19|website=CERN Courier|language=en-GB} ...t15=Charlotte |date=2023-07-19 |title=First Direct Observation of Collider Neutrinos with FASER at the LHC |journal=Physical Review Letters |volume=131 |issue=3 ...9 KB (1,270 words) - 01:16, 21 October 2024
- ...the observed flux of high energy [[cosmic rays]]. Since the highest energy neutrinos are produced from interactions of utlra-high-energy cosmic rays, the observ ...">{{Cite journal |last=Kajita |first=Takaaki |date=2010 |title=Atmospheric neutrinos and discovery of neutrino oscillations |journal=Proceedings of the Japan A ...16 KB (2,400 words) - 10:42, 10 February 2025
- ...se]] at early times.<ref>Longair (2006), p. 290</ref> Prior to decoupling, neutrinos were in [[thermal equilibrium]] with [[proton]]s, [[neutron]]s and [[electr ...resent-day direct detection.<ref name="forbes_neutrino"/> Even high energy neutrinos are [[neutrino detector|notoriously difficult to detect]], so the CNB may n ...11 KB (1,538 words) - 00:57, 28 August 2021
- Monitored neutrino beams are facilities for the production of [[Neutrino|neutrinos]] with unprecedented control of the flux of particles created inside and ou == Accelerator neutrinos == ...10 KB (1,521 words) - 12:57, 5 January 2024
- [[File:GlashowResonanceCrossSection.png|thumb|Cross sections between neutrinos and <sup>16</sup>O for W-boson production, compared to those for charged-cu ...process is considered for the detection and studies of high-energy cosmic neutrinos at the [[IceCube Neutrino Observatory|IceCube experiment]], at the [[ANTARE ...3 KB (397 words) - 18:51, 25 May 2024
- | title = A study of the scenario with nearly degenerate Majorana neutrinos | title = Bimaximal mixing of three neutrinos ...5 KB (704 words) - 15:56, 4 December 2024
- ...ial [[neutrino]] beam in which the flavor, flux and energy of the produced neutrinos are known with unprecedented precision. ...rs. DUNE and Hyper-Kamiokande are aimed at discovering [[CP violation]] in neutrinos observing a small difference between the probability of a muon-neutrino to ...8 KB (1,167 words) - 17:33, 14 December 2024
- ...with the [[cosmic neutrino background]] (CNB), which is comprised by relic neutrinos that were produced during the [[Big Bang]] and have much lower energies (10 {{See also|Supernova neutrinos}} ...15 KB (2,190 words) - 10:52, 8 February 2025
- ...universe, which produced a cosmic neutrino background of freely streaming neutrinos. An important consequence of neutrino decoupling is that the [[cosmic neutr ...ame [[Relativistic particle|non-relativistic]] (by comparison, photons and neutrinos decoupled while still relativistic and are known as "hot relics"). By calcu ...7 KB (1,065 words) - 16:29, 23 December 2024
- In 2014, RENO announced the observation of an unexpectedly large number of neutrinos with an energy of {{val|5|1|ul=MeV}}.<ref name=neutrino2014>{{Cite conferen ...4 KB (605 words) - 23:02, 29 May 2024
- {{Short description|Experiment investigating oscillation of neutrinos}} ...n]] of [[neutrino]]s from a nuclear reactor into light so-called [[sterile neutrinos]]. It was located at the [[Institut Laue–Langevin]] (ILL) in Grenoble, Fran ...14 KB (1,966 words) - 16:06, 13 June 2024
- ...ss]] of [[neutrino]]s. Astronomical searches investigate whether light and neutrinos emitted simultaneously from a distant source are arriving simultaneously on Since it is established that neutrinos possess mass, the speed of neutrinos of [[kinetic energy|kinetic energies]] ranging from [[electronvolt|MeV]] to ...27 KB (3,780 words) - 08:46, 16 May 2024
- Although "[[sterile neutrinos]]" are ''not'' included in the [[Standard Model]] and have ''not'' been con ...p|0}}}} interacts with ''all'' fermions will need an exception for sterile neutrinos inserted, if they are ever detected experimentally. ...34 KB (4,792 words) - 10:33, 1 March 2025
- ...clear Power Plant]] reactors as a neutrino source and measured the flux of neutrinos from them. To accomplish this, Double Chooz had a set of two detectors situ ...set to 350 keV, much lower than the 1.02 MeV expected of the electron anti-neutrinos.<ref name="arxiv2" /><ref name="arxiv3" /> ...14 KB (2,059 words) - 14:27, 12 June 2024
- ...ck-neutrinos-in-liquid-argon/|title=Sam Zeller receives DOE award to track neutrinos in liquid argon|first=Leah|last=Hesla|work=News at work|publisher=Fermilab| ...ald|date=September 29, 2021|first=Dave|last=Oberhelman|title='Rock star of neutrinos' to appear on 'Nova'}}</ref> ...10 KB (1,341 words) - 18:38, 28 March 2024
- For neutrinos and gamma rays, the departing particle gets almost all the energy, the frac If we take <math>M_p=0</math> for neutrinos and gamma rays, this simplifies to: ...8 KB (1,374 words) - 15:33, 27 November 2023
- 4 KB (512 words) - 11:38, 1 January 2025
- ...ee mass eigenstates of the left-helicity neutrinos and right-helicity anti-neutrinos each must have non-zero mass. ...15 KB (2,164 words) - 23:47, 15 November 2024
- {{Short description|Astronomical neutrinos produced during core-collapse supernova explosion}} ...igh Energy physics — PoS(ICHEP2020) |chapter=Core-Collapse Supernove Burst Neutrinos in DUNE |date=2021-04-15|language=en|publisher=SISSA Medialab|volume=390|pa ...37 KB (5,132 words) - 14:10, 4 October 2024