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相关概念视频

Detection of Black Holes01:10

Detection of Black Holes

1.7K
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 Magnetic Moment00:59

Atomic Nuclei: Nuclear Magnetic Moment

3.0K
All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
3.0K
Atomic Nuclei: Magnetic Resonance01:05

Atomic Nuclei: Magnetic Resonance

1.2K
The number of nuclear spins aligned in the lower energy state is slightly greater than those in the higher energy state. In the presence of an external magnetic field, as the spins precess at the Larmor frequency, the excess population results in a net magnetization oriented along the z axis. When a pulse or a short burst of radio waves at the Larmor frequency is applied along the x axis, the coupling of frequencies causes resonance and flips the nuclear spins of the excess population from the...
1.2K
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

1.1K
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
1.1K
Magnetic Fields01:27

Magnetic Fields

6.0K
A moving charge or a current creates a magnetic field in the surrounding space, in addition to its electric field. The magnetic field exerts a force on any other moving charge or current that is present in the field. Like an electric field, the magnetic field is also a vector field. At any position, the direction of the magnetic field is defined as the direction in which the north pole of a compass needle points.
A magnetic field is defined by the force that a charged particle experiences...
6.0K
Magnetic Field Lines01:19

Magnetic Field Lines

5.4K
The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
5.4K

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相关实验视频

Updated: May 1, 2026

High-Sensitivity Nuclear Magnetic Resonance at Giga-Pascal Pressures: A New Tool for Probing Electronic and Chemical Properties of Condensed Matter under Extreme Conditions
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High-Sensitivity Nuclear Magnetic Resonance at Giga-Pascal Pressures: A New Tool for Probing Electronic and Chemical Properties of Condensed Matter under Extreme Conditions

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在正常星系中强大的磁场在高红移的正常星系中强烈的磁场.

Martin L Bernet1, Francesco Miniati, Simon J Lilly

  • 1Department of Physics, ETH Zürich, Wolfgang-Pauli-Strasse 16, CH-8093 Zürich, Switzerland.

Nature
|July 18, 2008
PubMed
概括

早期的星系拥有强大的磁场,与今天的磁场相当. 这项研究将这些强大的银河磁场与早期宇宙中的正常星系联系起来,挑战了关于它们的起源和时间尺度的先前假设.

科学领域:

  • 天文学和天体物理学
  • 宇宙磁力宇宙磁力宇宙磁力
  • 银河系的进化 银河系的进化

背景情况:

  • 银河系中的磁场的起源和放大仍然不太清楚.
  • 动力发电机效应是种子磁场在宇宙时间上的放大假定机制.
  • 以前的研究表明,早期和当今星系的磁场强度相似,但它们的分布不清楚.

研究的目的:

  • 研究磁场在早期宇宙中的起源和分布.
  • 为了确定高磁场强度是否与正常星系或特定类星体环境有关.
  • 通过动力发电机效应来限制磁场放大时间尺度.

主要方法:

  • 分析遥远类星体的高分辨率光谱.
  • 测量旋转量 (RMs) 以追踪磁场强度.
  • RMs与Mg II吸收线的相关性,表明银河系光环环境.

主要成果:

  • 在高旋转量测量和类星体中强大的Mg II吸收线之间发现了明确的关联.
  • 二吸收线沿着视线追踪到类星体的正常星系的光环.
  • 这表明,当宇宙只有其当前年龄的三分之一时,正常星系中存在强大,有组织的磁场.

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Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement

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High-Sensitivity Nuclear Magnetic Resonance at Giga-Pascal Pressures: A New Tool for Probing Electronic and Chemical Properties of Condensed Matter under Extreme Conditions
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High-Sensitivity Nuclear Magnetic Resonance at Giga-Pascal Pressures: A New Tool for Probing Electronic and Chemical Properties of Condensed Matter under Extreme Conditions

Published on: October 10, 2014

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Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement
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Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement

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Optimizing Magnetic Force Microscopy Resolution and Sensitivity to Visualize Nanoscale Magnetic Domains

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结论:

  • 具有显著强度的有组织磁场与早期宇宙中的正常星系有关.
  • 这一发现挑战了这样一个观念,即这些场只会在以后发展,或者仅限于不寻常的银河系环境.
  • 结果为银河系动力发电机作用模型和宇宙磁性的演变提供了关键的约束.