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neutrino

[ noo-tree-noh, nyoo- ]

noun

, Physics.
, plural neu·tri·nos.
  1. any of the massless or nearly massless electrically neutral leptons. There is a distinct kind of neutrino associated with each of the massive leptons.


neutrino

/ njuːˈtriːnəʊ /

noun

  1. physics a stable leptonic neutral elementary particle with very small or possibly zero rest mass and spin 1 2 that travels at the speed of light. Three types exist, associated with the electron, the muon, and the tau particle
“Collins English Dictionary — Complete & Unabridged” 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

neutrino

/ no̅o̅-trē /

  1. Any of three electrically neutral subatomic particles with extremely low mass. These include the electron-neutrino, the muon-neutrino, and the tau-neutrino.
  2. ◆ The study of neutrinos that come to the earth as cosmic rays suggests that neutrinos can transform into each other in a process called neutrino oscillation . For this phenomenon to be theoretically possible, the three neutrinos must have distinct masses; for this reason, many scientists believe that they have mass.
  3. See Table at subatomic particle

neutrino

  1. An electrically neutral particle that is often emitted in the process of radioactive decay of nuclei . Neutrinos are difficult to detect, and their existence was postulated twenty years before the first one was actually discovered in the laboratory. Millions of neutrinos produced by nuclear reactions in the sun pass through your body every second without disturbing any atoms .
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Word History and Origins

Origin of neutrino1

< Italian (1933), equivalent to neutr ( o ) neuter, neutral + -ino -ine 2; coined by E. Fermi
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Word History and Origins

Origin of neutrino1

C20: from Italian, diminutive of neutrone neutron
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A Closer Look

Neutrinos were not observed until 1955, roughly a quarter of a century after the physicist Wolfgang Pauli first hypothesized their existence on theoretical grounds. Pauli was studying certain radioactive decay processes called beta decay , processes now known to involve the decay of a neutron into a proton and an electron. A certain amount of energy that was lost in these processes could not be accounted for. Pauli suggested that the energy was carried away by a very small, electrically neutral particle that was not being detected. (He originally wanted to name the particle a neutron but didn't publish the suggestion, and a few years later the particle we now know as the neutron was discovered and named in print. The Italian physicist Enrico Fermi then coined the term neutrino, which means “little neutron” in Italian.) Neutrinos are hard to detect because their mass, if they indeed have any, is extremely low, and they possess no electric charge; a chunk of iron a few light-years thick would absorb only about half of the neutrinos that struck it. Nevertheless, neutrinos can be detected, and three different types have been distinguished, each of which is associated with a particular lepton (the electron, the muon, and the taon) with which it is often paired in interactions involving the weak force. Recent analysis of neutrinos emanated by the Sun has suggested that each type of neutrino can spontaneously turn into one of the others in a process of neutrino oscillation, and for theoretical reasons this in turn would require that neutrinos have mass. If so, then despite their light weight, their abundance may in fact mean that neutrinos contribute significantly to the overall mass of the universe.
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Example Sentences

The simulations showed for the first time that, however briefly, even neutrinos can be trapped by the heat and density of the merger.

The collaboration doubled their neutrino data since their previous release four years ago, including adding a new low-energy sample of electron neutrinos.

Their estimations are consistent with a scenario in which the smaller kick imparted during the stellar collapse was not due to baryonic matter, which includes neutrons and protons, rather to so-called neutrinos.

The move effectively sends researchers back to the drawing board, and it bodes ill for plans to expand the gigantic IceCube neutrino detector at the pole.

The team was able to study more than 300,000 neutrinos.

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