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相关概念视频

Atomic Spectroscopy: Effects of Temperature01:27

Atomic Spectroscopy: Effects of Temperature

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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...
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Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

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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.
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Radioactive Decay and Radiometric Dating02:48

Radioactive Decay and Radiometric Dating

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Radioactivity is a spontaneous disintegration of an unstable nuclide and is a random process, as all the nuclei in the sample do not decay simultaneously. The number of disintegrations per unit time is called the activity (A), which is directly proportional to the number of nuclei in the sample. The decay constant (λ) is an average probability of decay per nucleus in unit time.
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Nuclear Fission02:50

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Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large...
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Nuclear Stability03:18

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Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively...
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Atomic Nuclei: Types of Nuclear Relaxation01:28

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Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers...
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Updated: May 15, 2025

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
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一个-229固态核钟的温度灵敏度

Jacob S Higgins1, Tian Ooi1, Jack F Doyle1

  • 1University of Colorado, NIST, JILA, and University of Colorado, Department of Physics, Boulder, Colorado 80309, USA.

Physical review letters
|April 7, 2025
PubMed
概括

研究人员测量了-229核转换在化晶体内的温度依赖的变化. 一个过渡显示最小的转移,表明稳定的固态光学时钟的潜力.

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科学领域:

  • 核光谱学是指核光谱学.
  • 量子时钟的使用方法
  • 固态物理 固态物理

背景情况:

  • 已经实现了低能-229核过渡的量子状态分辨率光谱.
  • 在化主体晶体中以千赫兹精度测量了五个电四极过渡.
  • 了解系统变化,如温度依赖,对于固态核时钟的性能至关重要.

研究的目的:

  • 测量-229核过渡的温度依赖性.
  • 为了研究未分割频率和电四极分裂的变化.
  • 为了确定未来固态光学时钟应用的有希望的过渡.

主要方法:

  • 对四个最强-229过渡的光谱测量.
  • 在化晶体中进行的实验,温度为150K,229K和293K.
  • 分析与电子密度和电场梯度相关的频率转移.

主要成果:

  • 观察到温度依赖的频率变化和四极分裂.
  • 电子密度下降,电场梯度和不对称性随着温度的增加.
  • 在m=±5/2→±3/2过渡中,在温度范围 (约. 0.4 kHz/K) 的时间.

结论:

  • m=±5/2→±3/2过渡的最小温度依赖使其成为固态光学钟的强有力的候选者.
  • 为了达到10-18的精度,需要在5μK以内的晶体温度稳定性.
  • 进一步研究核钟和系统的转移缓解是有必要的.