核结合能


核结合能(英语:Nuclear binding energy),又称原子能或核能,是由组成原子核的粒子之间发生的反应释放出的能量。原子能比化学反应中释放的热能要大将近5千万倍:铀核裂变的这种原子能释放形式约为200,000,000电子伏特(一种能量单位),而碳的燃烧这种化学反应能量仅放出4.1电子伏特。
1905年,阿尔伯特·爱因斯坦提出狭义相对论,之后作为推论,又提出质能方程E=mc²,(其中E=能量,m=质量,c=光速常量)。自此核能得到科学的解释和开发利用。
单词 | Nuclear binding energy |
释义 |
Nuclear binding energy
中文百科
核结合能![]() ![]() 核结合能(英语:Nuclear binding energy),又称原子能或核能,是由组成原子核的粒子之间发生的反应释放出的能量。原子能比化学反应中释放的热能要大将近5千万倍:铀核裂变的这种原子能释放形式约为200,000,000电子伏特(一种能量单位),而碳的燃烧这种化学反应能量仅放出4.1电子伏特。 1905年,阿尔伯特·爱因斯坦提出狭义相对论,之后作为推论,又提出质能方程E=mc²,(其中E=能量,m=质量,c=光速常量)。自此核能得到科学的解释和开发利用。
英语百科
Nuclear binding energy 核结合能![]() ![]() ![]() Nuclear binding energy is the energy that would be required to disassemble the nucleus of an atom into its component parts. These component parts are neutrons and protons, which are collectively called nucleons. The binding energy of nuclei is due to the attractive forces that hold these nucleons together and this is usually a positive number, since most nuclei would require the expenditure of energy to separate them into individual protons and neutrons. The mass of an atomic nucleus is usually less than the sum of the individual masses of the constituent protons and neutrons (according to Einstein's equation E=mc) and this 'missing mass' is known as the mass defect, and represents the energy that was released when the nucleus was formed. |
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