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相关概念视频

Subatomic Particles03:37

Subatomic Particles

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Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
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Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
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Atomic Nuclei: Nuclear Spin State Population Distribution01:14

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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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A substance that reaches superconductivity, a state in which magnetic fields cannot penetrate, and there is no electrical resistance, is referred to as a superconductor. In 1911, Heike Kamerlingh Onnes of Leiden University, a Dutch physicist, observed a relation between the temperature and the resistance of the element mercury. The mercury sample was then cooled in liquid helium to study the linear dependence of resistance on temperature. It was observed that, as the temperature decreased, the...
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Atomic Absorption Spectroscopy: Atomization Methods01:25

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Atomic Absorption Spectroscopy (AAS) atomizes samples through flame atomization or electrothermal atomization. Flame atomization typically involves a nebulizer and spray chamber assembly to combine the sample with a fuel–oxidant mixture, creating a fine aerosol mist that enters a burner. Typically, the fuel and oxidant are combined in an approximately stoichiometric ratio. However, for atoms that are easily oxidized, a fuel-rich mixture may be more advantageous. Only about 5% of the...
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Interference leads to systematic error in atomic absorption (AA) measurements by enhancing or diminishing the analytical signal or the background. These interferences can be grouped into three main categories: spectral interference, chemical interference, and physical interference.
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相关实验视频

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Angle-resolved Photoemission Spectroscopy At Ultra-low Temperatures
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制造和检测冷反原子的方法

M Amoretti1, C Amsler, G Bonomi

  • 1Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Università di Genova, 16146 Genova, Italy.

Nature
|October 9, 2002
PubMed
概括

研究人员为精确的CPT不变性测试创建了冷的抗原子. 检测这些低能反原子验证了基本粒子物理学的一个关键原则.

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科学领域:

  • 基本的粒子物理学的基础.
  • 反物质研究的研究.
  • 量子力学就是量子力学.

背景情况:

  • CPT不变性是标准模型的基石,在电荷联,平价和时间逆转下断言物理定律对称.
  • 迪拉克预测的反物质提供了一种途径,通过粒子-反粒子比较来实验测试CPT对称性.
  • 之前在CERN和费米实验室生产的反缺乏精密光谱所需的低能条件.

研究的目的:

  • 为了证明产生非常低能量的反原子.
  • 为了使用冷反原子进行CPT不变性的精确实验测试.
  • 建立一种研究反物质性质的新方法.

主要方法:

  • 在冷环境中捕获反质子和正电子.
  • 混合被困的抗粒子以形成中性抗抗原子.
  • 通过在成像粒子探测器中观察它们的灭绝特征,直接检测抗.

主要成果:

  • 成功生产了冷的反原子.
  • 一种适用于精度测量的方法的演示.
  • 观察到特有的灭绝签名,证实了反原子的检测.

结论:

  • 制造冷抗是可行的.
  • 这种技术为高精度的CPT测试打开了道路.
  • 进一步的研究可以以前所未有的准确性探索反物质的特性.