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相关概念视频

Photoluminescence: Applications01:14

Photoluminescence: Applications

Photoluminescence offers a wide range of applications due to its inherent sensitivity and selectivity. This technique allows for both direct and indirect analyses of the analyte. Direct quantitative analysis is possible when the analyte exhibits a favorable quantum yield for fluorescence or phosphorescence. However, an indirect analysis may be feasible if the analyte is not fluorescent or phosphorescent, or if the quantum yield is unfavorable. Indirect methods include reacting the analyte with...
Photoluminescence: Fluorescence and Phosphorescence01:23

Photoluminescence: Fluorescence and Phosphorescence

Photoluminescence is a process where a molecule absorbs light energy and re-emits it in the form of light. This phenomenon occurs when a substance absorbs photons, promoting its electrons to higher energy level excited states, followed by a relaxation process in which the electrons return to their original ground state energy levels and emit light. Photoluminescence is widely observed in various materials, including semiconductors, and organic and inorganic compounds.
A pair of electrons in a...
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...
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...
Nuclear Transmutation03:20

Nuclear Transmutation

Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed protons being...
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...

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相关实验视频

Updated: May 19, 2026

In Situ Measurement and Correlation of Cell Density and Light Emission of Bioluminescent Bacteria
05:52

In Situ Measurement and Correlation of Cell Density and Light Emission of Bioluminescent Bacteria

Published on: June 28, 2018

发光的超新星

Avishay Gal-Yam1

  • 1Department of Particle Physics and Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100, Israel. avishay.gal-yam@weizmann.ac.il

Science (New York, N.Y.)
|August 28, 2012
PubMed
概括
此摘要是机器生成的。

超发光超新星 (SLSNe) 是极其明亮的恒星爆炸. 最近的研究重点是了解它们巨大的亮度的起源,将它们分类为类型,如缺乏的SLSN-I.

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A Step Beyond BRET: Fluorescence by Unbound Excitation from Luminescence (FUEL)
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Bioluminescence-Based Tumor Quantification Method for Monitoring Tumor Progression and Treatment Effects in Mouse Lymphoma Models

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Last Updated: May 19, 2026

In Situ Measurement and Correlation of Cell Density and Light Emission of Bioluminescent Bacteria
05:52

In Situ Measurement and Correlation of Cell Density and Light Emission of Bioluminescent Bacteria

Published on: June 28, 2018

A Step Beyond BRET: Fluorescence by Unbound Excitation from Luminescence (FUEL)
07:04

A Step Beyond BRET: Fluorescence by Unbound Excitation from Luminescence (FUEL)

Published on: May 23, 2014

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科学领域:

  • 天文学和天体物理学
  • 太空爆炸 太空爆炸

背景情况:

  • 几个世纪以来,人们一直观察到超新星或恒星爆炸.
  • 超发光的超新星 (SLSNe) 是一个最近记录的子类,其亮度超过每秒7 × 1043 ergs.
  • SLSNe被分为放射性发电 (SLSN-R),富含气 (SLSN-II) 和缺乏气 (SLSN-I) 的类型.

研究的目的:

  • 为了调查SLSNe.极端亮度的物理起源.
  • 提供关于SLSNe的当前研究的全面概述.

主要方法:

  • 对累积的观测证据和理论模型的审查.
  • 基于光谱特性 (存在) 和亮度的SLSNe的分类.

主要成果:

  • SLSN-I (缺乏) 代表了最明亮的类别.
  • 比SLSN-R.更频繁地观察到SLSN-II和SLSN-I,而不是SLSN-R.
  • 驱动SLSNe亮度的物理机制仍然是一个活跃的研究领域.

结论:

  • 了解SLSNe的不同起源对于天体物理学至关重要.
  • 需要进一步的研究来充分解释这些宇宙事件的极端能量输出.