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neutron FÍS.

neutron absorber FÍS.

neutron cycle FÍS.

neutron density FÍS.

neutron flux FÍS.

neutron hardening FÍS.

neutron source FÍS.

thermal neutron FÍS.

neutron induced radioisotopes FÍS.

thermal velocity neutron FÍS.

Ejemplos monolingües (no verificados por la redacción de PONS)

inglés
The equation of state for a neutron star is still not known.
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This same method is used in one class of radioisotope-based laboratory neutron sources that produce 30 neutrons for every million particles.
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The neutrons are slowed down as they travel through the water.
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Neutrons are a key product of fusion reactions.
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He wrote scientific papers, textbooks and review articles on the use of neutron scattering.
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This assumption breaks down near supermassive objects such as black holes and neutron stars due to tidal effects.
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A system made up of only two neutrons is not bound, though the attraction between them is very nearly enough to make them so.
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In contrast, all proposed forms of neutron star core material are fluids and are extremely unstable at pressures lower than that found in stellar cores.
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Experimentally, it can be accessed most directly by inelastic neutron scattering.
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It is also easier for unstable nuclei to absorb neutrons when the neutrons are traveling at a certain speed.
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