核天体物理学
![太阳系里的元素丰度(从氢到铀).氢跟氦的丰度最高[14]](/uploads/202501/30/SolarSystemAbundances.svg4904.png)
![Abundances of the chemical elements in the Solar System. Hydrogen and helium are most common, residuals within the paradigm of the Big Bang.[9] The next three elements (Li, Be, B) are rare because they are poorly synthesized in the Big Bang and also in stars. The two general trends in the remaining stellar-produced elements are: (1) an alternation of abundance of elements according to whether they have even or odd atomic numbers, and (2) a general decrease in abundance, as elements become heavier. Within this trend is a peak at abundances of iron and nickel, which is especially visible on a logarithmic graph spanning fewer powers of ten, say between logA=2 (A=100) and logA=6 (A=1,000,000).](/uploads/202501/30/SolarSystemAbundances4904.png)
核天体物理学(nuclear astrophysics)是天体物理学和核物理学的交叉学科,主要研究的领域有恒星结构,天体质量与其寿命的关系等,并从中了解恒星如何产生能量,认识化学元素的起源和演变与,分析驱动天体物理现象的机制。
单词 | Nuclear astrophysics |
释义 |
Nuclear astrophysics
中文百科
核天体物理学![]() ![]() 核天体物理学(nuclear astrophysics)是天体物理学和核物理学的交叉学科,主要研究的领域有恒星结构,天体质量与其寿命的关系等,并从中了解恒星如何产生能量,认识化学元素的起源和演变与,分析驱动天体物理现象的机制。
英语百科
Nuclear astrophysics 核天体物理学![]() Nuclear astrophysics is an interdisciplinary branch of physics involving close collaboration among researchers in various subfields of nuclear physics and astrophysics, with significant emphasis in areas such as stellar modeling, measurement and theoretical estimation of nuclear reaction rates, cosmology, cosmochemistry, gamma ray, optical and X-ray astronomy, and extending our knowledge about nuclear lifetimes and masses. In general terms, nuclear astrophysics aims to understand the origin of the chemical elements and the energy generation in stars. |
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