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Detection of Black Holes01:10

Detection of Black Holes

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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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Radiation: Applications01:17

Radiation: Applications

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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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Updated: May 5, 2026

How to Create and Use Binocular Rivalry
14:34

How to Create and Use Binocular Rivalry

Published on: November 10, 2010

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设计黑色镜子的设计

Ronald R Willey

    Applied optics
    |June 10, 2024
    PubMed
    概括

    黑色镜子,也称为总吸收器,旨在吸收特定波长带内的所有光线,与中性密度 (ND) 过器不同. 设计这些先进的光学涂层需要仔细考虑薄金属和介电层.

    科学领域:

    • 光学和材料科学 材料科学
    • 纳米技术和薄膜光学

    背景情况:

    • 黑色镜子或总吸收器的功能与中性密度 (ND) 过器不同,通过将反射率最小化到接近零.
    • 它们在特定波长频段实现了近乎完美的吸收,与控制发射率的ND过器不同.

    研究的目的:

    • 讨论程序并提供关于设计黑色镜子的额外视角.
    • 突出金属和介电层在实现总吸收方面的关键作用.

    主要方法:

    • 使用金属层来实现高吸收能力.
    • 采用介电层来设计增加吸收的干扰效应.
    • 解决与非常薄的金属层及其不同折射率相关的设计挑战.

    主要成果:

    • 黑色镜子的设计程序的演示.
    • 探索通过干扰使吸收层最大化电场强度的方法.
    • 考虑专门的软件来处理厚度取决于光学性能的薄金属层.

    结论:

    • 有效的黑镜设计需要吸收性金属层和增强干扰的介电层的组合.
    • 由于超薄金属薄膜的独特光学特性,设计过程需要专门的方法.

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  • 进一步介绍了黑镜设计方法的进一步见解.