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相关概念视频

¹H NMR: Long-Range Coupling01:27

¹H NMR: Long-Range Coupling

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The coupling interactions of nuclei across four or more bonds are usually weak, with J values less than 1 Hz. While these are usually not observed in spectra, the presence of multiple bonds along the coupling pathway can result in observable long-range coupling.
In alkenes, spin information is communicated via σ–π overlap, as seen in allylic (four-bond) and homoallylic (five-bond) couplings. These coupling interactions are stronger when the σ bond is parallel to the alkene...
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Detection of Black Holes01:10

Detection of Black Holes

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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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Space-Time Curvature and the General Theory of Relativity01:17

Space-Time Curvature and the General Theory of Relativity

4.2K
In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of...
4.2K
Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

2.3K
In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
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Spin–Spin Coupling: Two-Bond Coupling (Geminal Coupling)01:20

Spin–Spin Coupling: Two-Bond Coupling (Geminal Coupling)

1.6K
Two NMR-active nuclei bonded to a central atom can be involved in geminal or two-bond coupling. Geminal coupling is commonly seen between diastereotopic protons in chiral molecules and unsymmetrical alkenes, among others.
The central atom need not be NMR-active because its electrons are affected by the electron polarization of the spin-active atoms. However, spin information is transmitted less effectively than in one-bond coupling, and 2J values are usually weaker than 1J values. The energy of...
1.6K
Spin–Spin Coupling: Three-Bond Coupling (Vicinal Coupling)01:22

Spin–Spin Coupling: Three-Bond Coupling (Vicinal Coupling)

1.5K
Vicinal or three-bond coupling is commonly observed between protons attached to adjacent carbons. Here, nuclear spin information is primarily transferred via electron spin interactions between adjacent C‑H bond orbitals. This generally favors the antiparallel arrangement of spins, so 3J values are usually positive.
The extent of coupling depends on the C‑C bond length, the two H‑C‑C angles, any electron-withdrawing substituents, and the dihedral angle between the involved orbitals. The...
1.5K

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相关实验视频

Updated: Jan 18, 2026

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

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评估非最小合的宇宙学证据

William J Wolf1, Carlos García-García1, Theodore Anton1,2

  • 1University of Oxford, Astrophysics, DWB, Keble Road, Oxford OX1 3RH, United Kingdom.

Physical review letters
|September 10, 2025
PubMed
概括

有证据表明,不断演变的暗能量可能驱动宇宙加速. 数据支持标量场的凸潜在能量 (五质) 和与重力的非最小合,但这与第五力观测相矛盾.

科学领域:

  • 宇宙学的宇宙学是什么?
  • 理论物理 理论物理

背景情况:

  • 观测数据显示,与标准的寒冷暗物质Lambda模型有所差异.
  • 这些偏差表明,存在着不断演变的暗能量,可能是由被称为五官的宇宙学标量场驱动的.

研究的目的:

  • 评估观察证据,证明存在一个驱动宇宙加速的标量场.
  • 为了研究这个标量场的潜在能量及其与重力的合的特性.

主要方法:

  • 对观测数据的分析,以测试宇宙学模型.
  • 使用贝叶斯因子进行统计分析,以确定不同理论场景的偏好.

主要成果:

  • 数据支持凸的潜在能量为精华 (d^2V/dφ^2 < 0).
  • 强有力的证据 (log(B) =7.34±0.6) 支持一个与重力的非最小合的标量场.
  • 这种非最小的合预测了时间变化的引力常数和第五力.

结论:

  • 如果精华驱动宇宙加速,它的潜在能量必须是的.
  • 对非最小合的强烈偏好意味着可观察到的第五力,这些力没有被检测到.
  • 这表明,要么在较小的尺度上需要新的物理学,要么精华是宇宙加速的不太可能的解释.

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