相关实验视频
Updated: May 24, 2025

10:37
Spatial Separation of Molecular Conformers and Clusters
Published on: January 9, 2014
8.9K
选择后转移了在原子束中的过渡频率
Jin-Lu Wen1, Jia-Dong Tang2, Ya-Nan Lv2
1State Key Laboratory of Molecular Reaction Dynamics, Department of Chemical Physics, University of Science and Technology of China, Hefei 230026, China.
Science advances
|February 28, 2025
概括
这项研究揭示了光谱中的后选择引入了频率转移. 纠正这种偏差可以提供精确的过渡频率,这可能会挑战莱普顿的普遍性.
科学领域:
- 原子物理 原子物理
- 量子电动力学 量子电动力学
- 频谱学是一种光谱学.
背景情况:
- 后选择 (PS) 可以放大弱信号,但可能会偏差精度测量.
- 光谱对于基础物理测试至关重要.
研究的目的:
- 研究PS对23S - 23P过渡的精密光谱学的影响.
- 确定PS对测量过渡频率的影响.
- 获得对He4进行更正的,高精度的过渡频率.
主要方法:
- 利用原子束对 (He) 进行精密光谱.
- 直接观察并量化了基于位置的PS引起的频率转移.
- 对测量过渡频率进行了校正.
主要成果:
- 观察到一个显著的选择后诱导的频率转移大约为-55 kHz.
- 确定了对He的修正过渡频率: 276,764,094,712.45 ± 0.86 kHz.
- 导出二次核电荷半径的差异,显示与离子离子数据的偏差.
结论:
- 选择后引入了精确原子光谱学中可测量的偏差.
- 修正后的频率为He的23S1 - 23P0过渡提供了更准确的值.
- 核电荷半径的差异可能表明标准模型之外的新物理学,可能会挑战莱普顿的普遍性.
相关概念视频
Atomic Nuclei: Nuclear Spin State Population Distribution
911
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
911
The Bohr Model
50.3K
Following the work of Ernest Rutherford and his colleagues in the early twentieth century, the picture of atoms consisting of tiny dense nuclei surrounded by lighter and even tinier electrons continually moving about the nucleus was well established. This picture was called the planetary model since it pictured the atom as a miniature “solar system” with the electrons orbiting the nucleus like planets orbiting the sun. The simplest atom is hydrogen, consisting of a single proton as...
50.3K
Atomic Spectroscopy: Effects of Temperature
269
Atomization, converting samples into gas-phase atoms and ions, is essential for atomic spectroscopy. The flame temperature required for atomization affects the efficiency of the atomic spectroscopic methods by increasing the atomization efficiency and the relative population of the excited and ground states.
At thermal equilibrium, the relative populations of excited and ground state atoms can be estimated using the Maxwell–Boltzmann distribution. For example, an increase in temperature...
At thermal equilibrium, the relative populations of excited and ground state atoms can be estimated using the Maxwell–Boltzmann distribution. For example, an increase in temperature...
269
π Electron Effects on Chemical Shift: Overview
1.0K
An applied magnetic field causes loosely bound π-electrons in organic molecules to circulate, producing a local or induced diamagnetic field over a large spatial volume. As the molecules tumble in solution, the field generated by π-electrons in spherical substituents results in a zero net field. However, the net field generated by π-electrons in non-spherical substituents is not zero. The effect of this induced field depends on the orientation of the molecule with respect to B0,...
1.0K
Inductive Effects on Chemical Shift: Overview
1.1K
The protons in unsubstituted alkanes are strongly shielded with chemical shifts below 1.8 ppm. Methine, methylene, and methyl protons appear at approximately 1.7, 1.2 and 0.7 ppm, while the proton signal from methane appears at 0.23 ppm. An electronegative substituent, such as chlorine, withdraws the electron density from the protons, increasing their chemical shift. Progressive substitution of the hydrogens in methane by chlorine shifts the proton signals increasingly downfield, to 3.05 ppm in...
1.1K
UV–Vis Spectroscopy: Molecular Electronic Transitions
1.3K
In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this...
1.3K

