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...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 ...

...u neutrinos). However, even these numbers are not absolutely conserved, as neutrinos of different generations can [[quantum superposition|mix]]; that is, a neut ...awa matrix]] (CKM matrix). This matrix is analogous to the PMNS matrix for neutrinos, and quantifies flavour changes under charged weak interactions of quarks. ...

...f the Standard Model for neutrino oscillations which do not assume massive neutrinos, such as [[Lorentz-violating neutrino oscillations]]. |title=Neutrinos, Grand Unification and Leptogenesis ...

...timately to photons for neutral pions, and photons, positrons, and various neutrinos for positive pions. Neutrons also decay to similar products, so that ultima ...s |first3=A. |title=Ultra–High‐Energy Neutrino Scattering onto Relic Light Neutrinos in the Galactic Halo as a Possible Source of the Highest Energy Extragalact ...

In [[neutrino]]–nucleon scattering, neutrinos couple only via the axial current, thus accessing different nucleon structu ...

|title=High-energy cosmic rays and neutrinos from semirelativistic hypernovae ...

...stead it satisfies {{math|1={{mathcal|P}}{{i sup|4}} = 1}} so the Majorana neutrinos would have intrinsic parities of {{math|±''i''}}. ...

If neutrinos are [[Majorana particle]]s, a larger EDM (around {{val|e=-33|u=''e''⋅cm}}) ...

...p.201600050|arxiv=1610.01543|date=2016 |s2cid=118676940}}</ref> and 1.8 eV neutrinos are needed in clusters.<ref>{{Cite journal|title=Dirac neutrino mass from a ...

* [[Quarks]] and [[leptons]] (including [[electrons]] and [[neutrinos]]), which make up what is classically known as [[matter]], are all fermions ...

...d test for. To illustrate the point, an experiment to test for the mass of neutrinos or the decay of protons (small departures from the model) is more likely to ...

...arge-scale structure|large-scale structure]] of the universe. Other than [[neutrinos]], a form of [[hot dark matter]], dark matter has not been detected directl ...rinos rarely interact with anything, and are consequently rarely observed. Neutrinos stream throughout the universe but rarely interact with normal matter.<ref> ...

...can in principle destroy matter and convert all the energy of matter into neutrinos and usable energy, but it is normally extraordinarily slow. It was later sh ...

{{Main|Beta decay#Neutrinos}} ...

...rgy equivalence|mass–energy]] of a [[muon neutrino]]<ref>{{cite book|title=Neutrinos in physics and astrophysics: from 10–33 to 1028 cm: TASI 98 : Boulder, Colo ...

...ass through normal matter unimpeded and undetected.<ref>{{cite book |title=Neutrinos |author=Close, Frank |year=2010 |publisher=[[Oxford University Press]] |edi ...

...sed for this purpose. In particular, it is thought that ultra-high energy neutrinos in seawater can be detected acoustically.<ref>S. Bevan, S. Danaher, J. Perk ...