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相关概念视频

Physical Pendulum01:06

Physical Pendulum

When a rigid body is hanging freely from a fixed pivot point and is displaced, it oscillates similar to a simple pendulum and is known as a physical pendulum. The period and angular frequency of a physical pendulum are obtained by using the small-angle approximation and drawing parallels with a spring-mass system. The small-angle approximation (sinθ=θ) is valid up to about 14°.
When dealing with complicated systems, the mass moment of inertia is an important parameter, as it describes the mass...
Torsional Pendulum01:09

Torsional Pendulum

A torsional pendulum involves the oscillation of a rigid body in which the restoring force is provided by the torsion in the string from which the rigid body is suspended. Ideally, the string should be massless; practically, its mass is much smaller than the rigid body's mass and is neglected.
As long as the rigid body's angular displacement is small, its oscillation can be modeled as a linear angular oscillation. The amplitude of the oscillation is an angle. The role of mass is played by the...
Assessment of radial pulse01:11

Assessment of radial pulse

Assessment of Radial Pulse
The radial pulse, located at the wrist, is often the preferred site for assessing peripheral pulse because of its accessibility and dependability. The process of determining the radial pulse involves several steps:
Faraday Disk Dynamo01:23

Faraday Disk Dynamo

A Faraday disk dynamo is a DC generator, producing an emf that is constant in time. It consists of a conducting disk that rotates with a constant angular velocity in the magnetic field, perpendicular to the disk's plane. The rotation of the disk causes a change in magnetic flux, which induces an emf, causing opposite charges to develop on the rim and in the center of the disk. The polarity of the induced emf can be determined by the direction of the magnetic field and the direction of the...
Generating Electromagnetic Radiations01:10

Generating Electromagnetic Radiations

The German physicist Heinrich Hertz (1857–1894) was the first to generate and detect certain types of electromagnetic waves in the laboratory. Starting in 1887, he performed a series of experiments that confirmed the existence of electromagnetic waves and verified that they travel at the speed of light. Hertz used an alternating-current RLC (resistor-inductor-capacitor) circuit that resonated at a known frequency and connected it to a loop of wire. High voltages induced across the gap in the...
Electric Generator: Alternator01:25

Electric Generator: Alternator

Electric generators induce an emf by rotating a coil in a magnetic field. A simple alternator is an AC generator that creates electrical energy that varies sinusoidally with time. A simple alternator consists of a conducting loop that is placed inside a uniform magnetic field. The loop is connected to split rings connected to the external circuit with the help of brushes.
The magnetic flux passing through the coil varies sinusoidally as the loop rotates inside the magnetic field. This...

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相关实验视频

Updated: Jul 12, 2026

20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier
10:17

20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier

Published on: July 12, 2017

二进制脉冲星PSR 1913 + 16:其起源的模型

H M Van Horn, S Sofia, M P Savedoff

    Science (New York, N.Y.)
    |May 30, 1975
    PubMed
    概括

    这项研究模拟了二进制脉冲星PSR 1913 + 16,表明一个中子星脉冲星和一个矮伴侣. 观测数据约束系统参数,包括质量和轨道倾斜.

    科学领域:

    • * 天文学和天体物理学
    • * * 紧的对象 紧的对象
    • * 二进制系统 二进制系统

    背景情况:

    • *PSR 1913 + 16 是一个拥有现有观测数据的二进制脉冲星系统.
    • * 用进化考虑来建模系统的组件.

    研究的目的:

    • *为二进制脉冲星系统PSR 1913 + 16开发一个明确的模型.
    • * 确定脉冲星及其伴星的性质和特性.

    主要方法:

    • *对PSR1913 + 16的现有观测数据的分析.
    • * 应用进化模型来限制系统参数.
    • *用于估计脉冲星属性的磁双极模型.

    主要成果:

    • * 脉冲星被确定为一个中子星,接近上限质量 (1.2太阳质量).
    • *伴星可能是一个退化的矮星,质量接近上限 (0.25-1.0太阳质量).
    • *估计脉冲星年龄~4x10^4年,周期变化速率~2ns/天,磁场~1/3的脉冲星.

    结论:

    • * 衍生模型为PSR 1913 + 16提供了一致的解释.

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    A Basic Positron Emission Tomography System Constructed to Locate a Radioactive Source in a Bi-dimensional Space

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  • * 未来精确测量脉冲星周期变化和搜索超新星残骸将测试该模型.