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相关概念视频

Mass Spectrometry: Isotope Effect01:13

Mass Spectrometry: Isotope Effect

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Most elements exist in nature as a mixture of isotopes. The isotopes differ in weight due to their respective number of neutrons. The molecular weight of a molecule is different depending on the specific isotope of its elements involved. As a result, the mass spectrum of the molecule exhibits peaks from the same fragment at multiple positions. The positions of these mass signals depend on the difference between the molecular mass. Furthermore, the intensity of these signals is dependent on the...
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Atomic Mass01:52

Atomic Mass

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Atoms — and the protons, neutrons, and electrons that compose them — are extremely small. For example, a carbon atom weighs less than 2 × 10−23 g. When describing the properties of tiny objects such as atoms, we use appropriately small units of measure, such as the atomic mass unit (amu). The amu was originally defined based on hydrogen, the lightest element, then later in terms of oxygen. Since 1961, it has been defined with regard to the most abundant isotope of...
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High-Resolution Mass Spectrometry (HRMS)01:15

High-Resolution Mass Spectrometry (HRMS)

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The resolution of a mass spectrometer depends on the efficiency of separating ions with different ion masses. The mass of an atom is approximated to the sum of the masses of protons and neutrons inside, considering the masses of protons and neutrons as equal. However, the masses of the proton (1.6726 × 10−24 g) and neutron (1.6749 × 10−24 g) are not truly equal. There is a minor error in the expression of atomic masses relative to the simplest atom of hydrogen. For...
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Atomic Radii and Effective Nuclear Charge03:08

Atomic Radii and Effective Nuclear Charge

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The elements in groups of the periodic table exhibit similar chemical behavior. This similarity occurs because the members of a group have the same number and distribution of electrons in their valence shells.
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Gravitation Between Spherically Symmetric Masses01:14

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The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.
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Isotopes01:12

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Elements have a set number of protons that determines their atomic number (Z). For example, all atoms with eight protons are oxygen; however, the number of neutrons can vary for atoms of the same element. The sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are called isotopes. Elements can have multiple isotopes, for example, carbon-12, carbon-13, and carbon-14.
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相关实验视频

Updated: Jun 17, 2025

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
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超出10^{20} eV的宇宙射线的同变性有利于它们的重质量组成.

R U Abbasi1, Y Abe2, T Abu-Zayyad1,3

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Physical review letters
|August 9, 2024
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概括

我们使用天空分布数据估计了超高能宇宙射线 (UHECR) 的组成. 结果表明,在非常高的能量下重的组成,在较低的能量下可能更轻,这取决于银河系外磁场.

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科学领域:

  • 天体物理学 天体物理学
  • 粒子物理学 粒子物理学

背景情况:

  • 超高能宇宙射线 (UHECR) 是能量超过1018 eV的粒子.
  • 了解UHECR的组成对于识别它们的来源和传播机制至关重要.

研究的目的:

  • 估计10eEV以上的能量时注入的UHECR的质量组成.
  • 研究银河系外磁场 (EGMF) 对UHECR组成估计的影响.

主要方法:

  • 分析了望远镜阵列表面探测器观察到的UHECR事件的能源依赖的天空分布.
  • 将UHECR事件分布与局部宇宙的大规模结构进行比较.
  • 模拟不同强度的银河系外和银河系磁场的场景.

主要成果:

  • 一个相对较重的注射组合被推断为大约10 EeV,变得更轻到100 EeV.
  • 在能量超过100 EeV的UHECR组合被发现是非常重的,即使有强大的EGMF.
  • 如果存在强大的EGMF,则在较低的能量下可能会产生更轻的组成;银河系磁场的不确定性具有主导作用.

结论:

  • 注射的UHECR成分显示出显著的能源依赖.
  • 银河系外磁场在解释UHECR组成方面起着至关重要的作用,特别是在较低的能量下.
  • 观察到的UHECR很可能源自不同元素组成的混合来源.