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arXiv 0908.3275nucl-thastro-ph.SRnucl-exphysics.hist-phphysics.pop-ph
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核反应

Nuclear Reactions

C. A. Bertulani

摘要:

核反应在核反应堆中产生能量,在恒星中,并且负责宇宙中所有比氢重的元素的存在。核反应表示原子核之间以及原子核与其他基本粒子(如电子和光子)之间的反应。本章简要介绍了守恒定律和基本物理量的定义,然后对具体情况作了更详细的说明:(a)复合核的形成和衰变;(b)直接反应;(c)光子和电子散射;(d)重离子碰撞;(e)夸克-胶子等离子体的形成;(f)热核反应;(g)与放射性核束的反应。必要时,引入基本方程以帮助理解这些反应的一般性质。发表于Wiley Encyclopedia of Physics,ISBN-13:978-3-527-40691-3 - Wiley-VCH,Berlin,2009。

英文摘要:

Nuclear reactions generate energy in nuclear reactors, in stars, and are responsible for the existence of all elements heavier than hydrogen in the universe. Nuclear reactions denote reactions between nuclei, and between nuclei and other fundamental particles, such as electrons and photons. A short description of the conservation laws and the definition of basic physical quantities is presented, followed by a more detailed account of specific cases: (a) formation and decay of compound nuclei; (b)direct reactions; (c) photon and electron scattering; (d) heavy ion collisions; (e) formation of a quark-gluon plasma; (f) thermonuclear reactions; (g) and reactions with radioactive beams. Whenever necessary, basic equations are introduced to help understand general properties of these reactions. Published in Wiley Encyclopedia of Physics, ISBN-13: 978-3-527-40691-3 - Wiley-VCH, Berlin, 2009.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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