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nuclear fusion reaction

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a nuclear reaction in which nuclei combine to form more massive nuclei with the simultaneous release of energy

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A variety of nuclear fusion reactions take place in the cores of stars, that depend upon their mass and composition.
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It is used in nuclear fusion reactions, as a tracer in isotope geochemistry, and in specialized self-powered lighting devices.
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Stellar nucleosynthesis is the theory explaining the creation (nucleosynthesis) of chemical elements by nuclear fusion reactions between atoms within stars.
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In nuclear chemistry, nuclear fusion is a reaction in which two or more atomic nuclei are combined to form one or more different atomic nuclei and subatomic particles (neutrons or protons).
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It is this energy-releasing process that makes nuclear fusion in stars a self-sustaining reaction.
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Nuclei of masses greater than 56 cannot be formed by thermonuclear reactions (i.e. by nuclear fusion), but can be formed by neutron capture.
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In stars, it is formed by the nuclear fusion of hydrogen in proton-proton chain reactions and the CNO cycle, part of stellar nucleosynthesis.
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Hydrogen plays a vital role in powering stars through the proton-proton reaction and the CNO cycle of nuclear fusion.
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The transmutation of lithium atoms to helium in 1932 was the first fully man-made nuclear reaction, and lithium deuteride serves as a fusion fuel in staged thermonuclear weapons.
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First, in the Sun's core, hydrogen is converted into helium through nuclear fusion, in particular the p–p chain, and this reaction converts some mass into energy in the form of gamma ray photons.
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Since 56Ni (14 alpha particles) is easily produced from lighter nuclei in the alpha process in nuclear reactions in supernovae (see silicon burning process), it is the endpoint of fusion chains inside extremely massive stars, since addition of another alpha particle, resulting in 60Zn, requires a great deal more energy.
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11 sinne gevind in 6 ms. Hulle kom uit baie bronne en word nie nagegaan nie.