Neutrinos no Dicionário de Francês-Inglês da Oxford-Hachette

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The initial collapse of degenerate cores is accelerated by beta decay, photodisintegration and electron capture, which causes a burst of electron neutrinos.
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These few solar neutrinos have the larger energies.
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The difference between the measured and expected arrival time of neutrinos (compared to the speed of light) was approximately.
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The proton and neutron making up deuterium can be dissociated through neutral current interactions with neutrinos.
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The energy spectrum of solar neutrinos is also predicted by solar models.
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Charged leptons can combine with other particles to form various composite particles such as atoms and positronium, while neutrinos rarely interact with anything, and are consequently rarely observed.
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The energy threshold for the detection of neutrinos therefore can be lower, and protonelectronproton solar neutrinos (with an energy of) can be observed.
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However, in a phenomenon known as neutrino flavor oscillation, neutrinos are able to oscillate among the three available flavors while they propagate through space.
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From this reaction, 86% of all solar neutrinos are produced.
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Protons carry quarks, but the electroweak theory was concerned only with the electrons and neutrinos, with nothing postulated about quarks.
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