neutrinos in English
The leptons consist of the charged electron, muon and tau, together with three electronically neutral particles - the electron neutrino , muon neutrinos and tau neutrinos.
Use "neutrinos" in a sentence
1. Thus oscillating neutrinos must have mass; but massive neutrinos need not oscillate.
2. However, because neutrinos change flavor as they travel, at least two of the types of neutrinos must have mass.
3. Neutrinos are famously Aloof particles, and questions remained over exactly how neutrinos transfer their energy to the star’s ordinary matter under the extreme conditions of a collapsing star
4. Instead they would produce gamma rays, neutrinos and antimatter such as positrons and antiprotons, Gondolo said.
5. And neutrinos you can detect by the signature they leave when they hit water molecules.
6. Only if neutrinos do have some mass, however small, can they oscillate from one type to another.
7. The next decade looks promising - especially for those who study the newly hot topic of neutrinos.
8. At any given time, up to # neutrinos per cubic centimeter are sharing the same space as we humans
9. At any given time... up to # neutrinos per cubic centimeter... are sharing the same space as we humans
10. At any given time... up to 100 neutrinos per cubic centimeter... are sharing the same space as we humans.
11. Take the recent question of whether neutrinos, a type of near-massless subatomic particle, can travel faster than light.
12. About a third of the mass energy of the proton-Antiproton pair becomes inaccessible in the form of energetic neutrinos.
13. But isotopes, particles of electricity, antimatter, neutrinos, the conversion of mass to energy -- that's E=mc^2 -- gamma rays, transmutation.
14. Feb 22, 2021: Astrophysicists propose that all high-energy cosmic neutrinos are born by quasars (Nanowerk News) Scientists of the P
15. About 1046 joules, approximately 10% of the star's rest mass, is converted into a ten-second burst of neutrinos which is the main output of the event.
16. 112.4 Axions from Astrophysical Sources 112.4.1 Stellarenergy-losslimits Low-massweakly-interactingparticles(neutrinos,gravitons,Axions,baryonicorleptonicgauge bosons, etc.) are produced in hot astrophysical plasmas, and can thus transport energy out of stars
17. Actually, if you just look at your thumbnail -- about a square centimeter -- there are something like 60 billion neutrinos per second from the sun, passing through every square centimeter of your body.
18. 13 hours ago · The particles and Antiparticles of the Standard Model of particle physics are exactly in line with [+] what experiments require, with only massive neutrinos providing a difficulty and requiring
19. The KM3NeT-It site, at a depth of 3400 m, hosts the ARCA (Astroparticle Research with Cosmics in the Abyss) detector, with more widely spaced DOMs optimised for detecting high-energy cosmic neutrinos in the TeV–PeV range.
20. The KM3NeT-Fr site, at a depth of 2475 m, hosts the ORCA (Oscillation Research with Cosmics in the Abyss) detector, a more compact array with more closely spaced sensors optimised for atmospheric neutrinos in the GeV range.
21. When a low-energy electron Annihilates a low-energy positron (antielectron), the most probable is the creation of two or more photons, since the only other final-state Standard Model particles that electrons and positrons carry enough mass-energy to produce are neutrinos, which are approximately 10,000 times less likely to produce, and the creation of only one photon is
22. In order to prove this, scientists are working to detect "neutrinoless double-beta decay" - a situation in which natural decay of Tellurium dioxide crystals results in neutrinos giving away photons, electrons, and Antineutrons.In this case, if the particle really acts as its own antimatter, the antineutrinos will cancel each other out and make up a "neutrinoless" decay, with only 2.5