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相关概念视频

Detection of Black Holes01:10

Detection of Black Holes

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...
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

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 velocity with the...
Computed Tomography01:10

Computed Tomography

Tomography refers to imaging by sections. Computed tomography (CT) is a non-invasive imaging technique that uses computers to analyze several cross-sectional X-rays to reveal minute details about structures in the body.
The technique was invented in the 1970s and is based on the principle that as X-rays pass through the body, they are absorbed or reflected at different levels. In the technique, a patient lies on a motorized platform while a computerized axial tomography (CAT) scanner rotates...
Nuclear Fusion02:45

Nuclear Fusion

The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Cylinders in Three-Dimensional Space01:28

Cylinders in Three-Dimensional Space

A cylindrical surface is generated when a two-dimensional profile curve is translated along a straight line in three-dimensional space. The translated copies of the curve form a surface composed of parallel rulings, each oriented in the same fixed direction. This construction allows many three-dimensional forms to be described using relatively simple planar equations.In Cartesian coordinates, a cylindrical surface is often recognized by an equation that omits one of the three variables. For...
Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...

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相关实验视频

Updated: Jul 12, 2026

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

构建黑洞:超级计算机电影院

S L Shapiro, S A Teukolsky

    Science (New York, N.Y.)
    |July 22, 1988
    PubMed
    概括

    一个新的计算机代码模拟了相对论恒星团,揭示了不稳定的星团如何崩成黑洞. 这种模拟可以解释类星体和活跃星系核的起源.

    科学领域:

    • 天体物理学 天体物理学
    • 计算物理 计算物理
    • 一般相对论一般相对论.

    背景情况:

    • 相对论星团由于强大的引力场和接近光速的速度而呈现复杂的动态.
    • 了解这些星团的演化对于天体物理现象至关重要.
    • 之前的模型在模拟这种极端条件时遇到了局限性.

    研究的目的:

    • 开发和利用一种新的计算机代码来模拟相对论星团的动态演变.
    • 为了调查不稳定的星团的灾难性崩.

    主要方法:

    • 开发一种新的计算机代码来解决爱因斯坦的广义相对论方程.
    • 超级计算机模拟以模拟相对论星团的行为.
    • 使用彩色图形实时可视化模拟结果.

    主要成果:

    • 该代码成功模拟了相对论星团的动态演变.
    • 证明不稳定的星团经历了灾难性的崩.
    • 模拟显示,黑洞的形成来自崩的星团.

    结论:

    • 开发的代码为研究极端天体物理环境提供了强大的工具.

    相关实验视频

    Last Updated: Jul 12, 2026

    Setting Limits on Supersymmetry Using Simplified Models
    07:46

    Setting Limits on Supersymmetry Using Simplified Models

    Published on: November 15, 2013

  • 不稳定的星团崩成超大质量黑洞可能解释类星体和活跃星系核的起源.
  • 实时可视化有助于理解复杂的天体物理过程.