相关实验视频
Updated: Jan 19, 2026
02:13
Mass Defect, Nuclear Binding Energy and Nuclear Stability
14.7K
核时钟过渡的能量
Benedict Seiferle1, Lars von der Wense2, Pavlo V Bilous3
1Ludwig-Maximilians-University Munich, Garching, Germany. benedict.seiferle@physik.uni-muenchen.de.
Nature
|September 13, 2019
概括
研究人员精确地测量了-229同位体的能量, 这对于开发核光学钟至关重要. 这一突破为超精确的计时和物理学中的新应用铺平了道路.
科学领域:
- 核物理
- 原子物理
- 测量学
背景情况:
- -229 (229mTh) 的第一个激发异构状态是核光学时钟的有希望的候选者,因为它的激发能量低,辐射寿命长.
- 由于对229mTh能量的不精确知识,核钟的开发在地测和基本恒定研究中受到阻碍.
- 目前基于电子外的原子钟有其局限性,
研究的目的:
- 以高精度直接测量229mTh异构体状态到其基本状态的过渡能量.
- 为激光光谱应用确定与此核过渡相对应的波长.
- 推进精确计量技术,并使精确的核光学时钟的开发成为可能.
主要方法:
- 在中性229mTh原子的衰变过程中发出的内部转换电子的光谱.
- 直接测量过渡能量,不确定度为0.17电子伏.
- 使用测量的能量计算过渡波长.
主要成果:
- 用0.17 eV的标准偏差不确定性测量了229mTh的过渡能量.
- 能量对应于149.7 ± 3.1纳米的过渡波长.
- 这种波长可以通过使用高波生成的激光谱来获取.
结论:
- 精确测量229mTh的过渡能量使得高分辨率的激光光谱能够对核进行测量.
- 这些发现是朝着发展具有前所未有的精度的核光学时钟迈出的关键一步.
- 这项研究结合了核和原子物理学, 显著提升了精度计量学.
相关概念视频
Nuclear Binding Energy
14.7K
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound...
14.7K
Properties of Transition Metals
29.6K
Transition metals are defined as those elements that have partially filled d orbitals. As shown in Figure 1, the d-block elements in groups 3–12 are transition elements. The f-block elements, also called inner transition metals (the lanthanides and actinides), also meet this criterion because the d orbital is partially occupied before the f orbitals.
29.6K
Energy Diagrams, Transition States, and Intermediates
20.3K
Free-energy diagrams, or reaction coordinate diagrams, are graphs showing the energy changes that occur during a chemical reaction. The reaction coordinate represented on the horizontal axis shows how far the reaction has progressed structurally. Positions along the x-axis close to the reactants have structures resembling the reactants, while positions close to the products resemble the products. Peaks on the energy diagram represent stable structures with measurable lifetimes, while...
20.3K
Phase Transitions
22.6K
Whether solid, liquid, or gas, a substance's state depends on the order and arrangement of its particles (atoms, molecules, or ions). Particles in the solid pack closely together, generally in a pattern. The particles vibrate about their fixed positions but do not move or squeeze past their neighbors. In liquids, although the particles are closely spaced, they are randomly arranged. The position of the particles are not fixed—that is, they are free to move past their neighbors to...
22.6K
Nuclear Fusion
33.7K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
33.7K
Ionization Energy
43.0K
The amount of energy required to remove the most loosely bound electron from a gaseous atom in its ground state is called its first ionization energy (IE1). The first ionization energy for an element, X, is the energy required to form a cation with 1+ charge:
43.0K