Jove
Visualize
联系我们
JoVE
x logofacebook logolinkedin logoyoutube logo
关于 JoVE
概览领导团队博客JoVE 帮助中心
作者
出版流程编辑委员会范围与政策同行评审常见问题投稿
图书馆员
用户评价订阅访问资源图书馆顾问委员会常见问题
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experiments存档
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教师资源中心教师网站
使用条款与条件
隐私政策
政策

相关概念视频

Detection of Black Holes01:10

Detection of Black Holes

2.1K
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...
2.1K
¹H NMR: Interpreting Distorted and Overlapping Signals01:02

¹H NMR: Interpreting Distorted and Overlapping Signals

985
Spin systems where the difference in chemical shifts of the coupled nuclei is greater than ten times J are called first-order spin systems. These nuclei are weakly coupled, and their chemical shifts and coupling constant can generally be estimated from the well-separated signals in the spectrum.
As Δν decreases and the signals move closer, the doublets appear increasingly distorted. The intensities of the inner lines increase at the cost of those of the outer lines as the signals are...
985
¹³C NMR: ¹H–¹³C Decoupling01:04

¹³C NMR: ¹H–¹³C Decoupling

992
The probability of having two carbon-13 atoms next to each other is negligible because of the low natural abundance of carbon-13. Consequently, peak splitting due to carbon-carbon spin-spin coupling is not observed in spectra. However, protons up to three sigma bonds away split the carbon signal according to the n+1 rule, resulting in complicated spectra.
A broadband decoupling technique is used to simplify these complex, sometimes overlapping, signals. Broadband decoupling relies on a...
992
Difference from Background: Limit of Detection01:05

Difference from Background: Limit of Detection

5.2K
The limit of detection (LOD) is the smallest amount of analyte that can be distinguished from the background noise. The LOD value corresponds to the concentration at which the analyte signal is three times larger than the standard deviation of the blank signal. Below this value, the analyte signal cannot be differentiated from the background noise. It is calculated by dividing the calibration slope by 3 times the standard deviation of the blank signals.
The LOD indicates the presence or absence...
5.2K
Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

1.4K
Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...
1.4K
UV–Vis Spectrometers01:14

UV–Vis Spectrometers

1.2K
The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell.
1.2K

您也可能阅读

相关文章

通过共同作者、期刊和引用图与本文相关的文章。

排序
Same author

Spinning Black Holes in Astrophysical Environments.

Physical review letters·2025
Same author

Gravitational Waves from Binary Extreme Mass Ratio Inspirals: Doppler Shift and Beaming, Resonant Excitation, Helicity Oscillations, and Self-Lensing.

Physical review letters·2025
Same author

Late-Time Tails in Nonlinear Evolutions of Merging Black Holes.

Physical review letters·2025
Same author

Dynamical Response of Viscous Objects to Gravitational Waves.

Physical review letters·2025
Same author

Unstable Chords and Destructive Resonant Excitation of Black Hole Quasinormal Modes.

Physical review letters·2025
Same author

Environmental Effects in Extreme-Mass-Ratio Inspirals: Perturbations to the Environment in Kerr Spacetimes.

Physical review letters·2025

相关实验视频

Updated: May 22, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

3.4K

环境中的黑洞光谱:可检测性前景

Thomas F M Spieksma1, Vitor Cardoso1,2, Gregorio Carullo1,3

  • 1Niels Bohr Institute, Center of Gravity, Blegdamsvej 17, 2100 Copenhagen, Denmark.

Physical review letters
|March 14, 2025
PubMed
概括

环境影响不会显著改变未来引力波观测台检测到的黑洞回归信号. 只有Ringdown分析才能可靠地确定残余黑洞的质量和旋转.

更多相关视频

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

19.3K
Quantification of Hydrogen Concentrations in Surface and Interface Layers and Bulk Materials through Depth Profiling with Nuclear Reaction Analysis
14:11

Quantification of Hydrogen Concentrations in Surface and Interface Layers and Bulk Materials through Depth Profiling with Nuclear Reaction Analysis

Published on: March 29, 2016

26.5K

相关实验视频

Last Updated: May 22, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

3.4K
Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

19.3K
Quantification of Hydrogen Concentrations in Surface and Interface Layers and Bulk Materials through Depth Profiling with Nuclear Reaction Analysis
14:11

Quantification of Hydrogen Concentrations in Surface and Interface Layers and Bulk Materials through Depth Profiling with Nuclear Reaction Analysis

Published on: March 29, 2016

26.5K

科学领域:

  • 天体物理学 天体物理学
  • 引力波天文学 引力波天文学
  • 黑洞物理学 黑洞物理学

背景情况:

  • 二元黑洞合并的回归阶段提供了对残余黑洞特性的洞察.
  • 未来的引力波探测器的目标是更高的精度,潜在地检测环境影响.

研究的目的:

  • 为了研究黑洞环境对二进制凝聚后的回落信号的影响.
  • 评估仅用于残留黑洞特征的回归分析的可靠性.

主要方法:

  • 模拟二进制黑洞合并的环境效应.
  • 分析回信号,与真空对应器进行比较.
  • 对计划中的引力波探测器灵敏度进行评估.

主要成果:

  • 在天体物理环境中,对于计划的探测器灵敏度来说,环回信号与真空信号是不可区分的.
  • 发现光谱不稳定性在观察上与回归信号无关.
  • 与仅仅是灵感估计的偏差可能会提供对环境影响的见解.

结论:

  • 只有Ringdown的分析对于确定残余黑洞的红移质量和旋转非常有效.
  • 环境影响并不妨碍从回归数据中准确估计黑洞参数.
  • 未来的观测可以通过比较启发和回归数据来潜在地描述环境影响.