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

Focusing of Light in the Eye01:16

Focusing of Light in the Eye

2.5K
Light rays enter the eye through the cornea, a transparent dome-shaped tissue that is the eye's outermost layer. The cornea bends or refracts, light rays traveling to the pupil. The shape of the cornea determines how much of the light is bent and whether the image will be focused correctly on the retina at the back of the eye. Once the light has passed through both refraction layers, it converges into a single focal point onto a small area. This is where photoreceptors start transforming...
2.5K
Detection of Black Holes01:10

Detection of Black Holes

2.2K
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...
2.2K
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

1.9K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
1.9K
Gravity between Spherical Bodies01:27

Gravity between Spherical Bodies

8.3K
Newton's law of gravitation describes the gravitational force between any two point masses. However, for extended spherical objects like the Earth, the Moon, and other planets, the law holds with an assumption that masses of spherical objects are concentrated at their respective centers.
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
8.3K
Imaging Biological Samples with Optical Microscopy01:18

Imaging Biological Samples with Optical Microscopy

4.6K
Optical microscopy uses optic principles to provide detailed images of samples. Antonie van Leeuwenhoek designed the first compound optical microscope in the 17th century to visualize blood cells, bacteria, and yeast cells. In 1830, Joseph Jackson Lister created an essentially modern light microscope. The 20th century saw the development of microscopes with enhanced magnification and resolution.
In optical microscopy, the specimen to be viewed is placed on a glass slide and clipped on the stage...
4.6K
X-ray Imaging01:24

X-ray Imaging

5.4K
German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with...
5.4K

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

Post-hospitalized Health Conditions of Covid-19 patients: A Cross-sectional study in Bangladesh.

Mymensingh medical journal : MMJ·2026
Same author

Search for Light Pseudoscalar Bosons, Pair-Produced in Higgs Boson Decays in the Four-Electron Final State in Proton-Proton Collisions at sqrt[s]=13  TeV.

Physical review letters·2026
Same author

First Evidence for Mixing-Induced CP Violation in B_{s}^{0}→J/ψϕ(1020) Decays in pp Collisions at sqrt[s]=13  TeV.

Physical review letters·2026
Same author

Observation of Suppressed Charged-Particle Production in Ultrarelativistic Oxygen-Oxygen Collisions.

Physical review letters·2026
Same author

Measurement of D^{0} Meson Photoproduction in Ultraperipheral Heavy Ion Collisions.

Physical review letters·2026
Same author

Observation of tWZ Production at the CMS Experiment.

Physical review letters·2026
Same journal

Structure and Dynamics in the Magnetotails of Unmagnetized and Weakly Magnetized Bodies.

Space science reviews·2026
Same journal

Transport of Electrons in Tangled Magnetic Fields.

Space science reviews·2026
Same journal

The Solar Wind Electron (SWE) Instrument for the Interstellar Mapping and Acceleration Probe Mission.

Space science reviews·2026
Same journal

Inter-comparison of Mars Upper Atmosphere Neutral Density and Temperature Datasets from MAVEN.

Space science reviews·2026
Same journal

The Interstellar Mapping And Acceleration Probe High Energy (IMAP-Hi) Neutral Atom Imager.

Space science reviews·2026
Same journal

Origin and Evolution of the Galilean Satellites Within the Jovian System.

Space science reviews·2026
查看所有相关文章

相关实验视频

Updated: Jun 7, 2025

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

21.7K

银河系的强力透镜

A J Shajib1,2, G Vernardos3,4,5, T E Collett6

  • 1Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 USA.

Space science reviews
|November 11, 2024
PubMed
概括
此摘要是机器生成的。

星系中的强引力透镜 (SGL) 有助于探索星系进化,恒星质量和宇宙学. 本综述涵盖了SGL建模方法和关键发现,讨论了当前的限制和未来的改进.

关键词:
宇宙学参数 宇宙学参数星系:圆形和镜形,cD银河系:进化的演变星系:它们的结构.重力透镜:强大的重力透镜.

更多相关视频

Demonstration of a Hyperlens-integrated Microscope and Super-resolution Imaging
10:01

Demonstration of a Hyperlens-integrated Microscope and Super-resolution Imaging

Published on: September 8, 2017

7.7K
Simulating the Mechanics of Lens Accommodation via a Manual Lens Stretcher
05:14

Simulating the Mechanics of Lens Accommodation via a Manual Lens Stretcher

Published on: February 23, 2018

6.8K

相关实验视频

Last Updated: Jun 7, 2025

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

21.7K
Demonstration of a Hyperlens-integrated Microscope and Super-resolution Imaging
10:01

Demonstration of a Hyperlens-integrated Microscope and Super-resolution Imaging

Published on: September 8, 2017

7.7K
Simulating the Mechanics of Lens Accommodation via a Manual Lens Stretcher
05:14

Simulating the Mechanics of Lens Accommodation via a Manual Lens Stretcher

Published on: February 23, 2018

6.8K

科学领域:

  • 天体物理学 天体物理学
  • 宇宙学的宇宙学是什么?
  • 银河系动力学 银河系动力学

背景情况:

  • 星系尺度上的强引力透镜 (SGL) 是一个重要的天体物理工具.
  • 它可以研究圆星系质量结构,进化和恒星初始质量函数.
  • 此外,SGL对于测量宇宙学参数至关重要.

研究的目的:

  • 审查用于建模星系规模引力透镜的常用方法,重点关注成像数据.
  • 总结来自银河系尺度镜头的关键天体物理学和宇宙学发现.
  • 讨论SGL研究当前的局限性和未来的前景.

主要方法:

  • 描述用于建模透镜可观测的流行的技术.
  • 强调分析成像数据作为最有信息的可观测来源.
  • 已经确定的发现和方法的文献综合.

主要成果:

  • 银河系规模的引力透镜提供了对银河系质量分布和演变的洞察.
  • 它有助于限制恒星初始质量函数,并完善宇宙参数测量.
  • 自20世纪80年代以来,数据质量和建模方面取得了重大进展.

结论:

  • 银河系规模的引力透镜是天体物理学和宇宙学的强大,多功能工具.
  • 数据和方法的不断改进有望增强未来的应用.
  • 该审查强调了该领域的进展,并概述了未来研究的方向.