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相关概念视频

Atomic Structure01:33

Atomic Structure

All matter is composed of atoms, the smallest individual units of elements. Each atom is made up of three subatomic particles: protons, neutrons, and electrons. Together, these three particles account for the mass and the charge of an atom.The History of Atomic TheoryThe first person to propose that everything on Earth is made up of tiny particles was the Greek philosopher Democritus, around 450 B.C. He used the term atomos, Greek for “indivisible,” from which the modern term “atom” is derived.
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
Emission Spectra02:39

Emission Spectra

When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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...
Atomic Structure01:17

Atomic Structure

The Greek philosopher Democritus proposed that everything on Earth is made up of tiny particles called atomos, Greek for "indivisible," from which the modern term "atom" is derived. In the 19th century, John Dalton proposed the atomic theory that is still largely correct today. He put forth five postulates to explain how atoms made up the world around us. (1) All matter is composed of infinitely small particles or atoms. (2) All atoms of a given element are identical to one another and (3) are...
Hydrogen Bonds01:04

Hydrogen Bonds

A hydrogen bond is formed when a weakly positive hydrogen atom already bonded to one electronegative atom (for example, the oxygen in the water molecule) is attracted to another electronegative atom from another polar molecule, such as water (H2O), hydrogen fluoride (HF), or ammonia (NH3). The huge electronegativity difference between the H atom (2.1) and the atom to which it is bonded (4.0 for an F atom, 3.5 for an O atom, or 3.0 for an N atom), combined with the very small size of an H atom...

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相关实验视频

Updated: Jul 6, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
07:17

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

Published on: August 1, 2017

大爆炸后10亿年宇宙的中性分数.

J Stuart B Wyithe1, Abraham Loeb

  • 1School of Physics, The University of Melbourne, Parkville, Victoria 3010, Australia.

Nature
|February 27, 2004
PubMed
概括
此摘要是机器生成的。

早期的宇宙 早期的宇宙

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相关实验视频

Last Updated: Jul 6, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
07:17

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

Published on: August 1, 2017

Cryogenic Liquid Jets for High Repetition Rate Discovery Science
08:34

Cryogenic Liquid Jets for High Repetition Rate Discovery Science

Published on: May 9, 2020

Hydrogen Production and Utilization in a Membrane Reactor
10:00

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科学领域:

  • 宇宙学的宇宙学是什么?
  • 天体物理学 天体物理学
  • 早期宇宙研究 早期宇宙研究

背景情况:

  • 星际介质 (IGM) 中的的电离状态为早期宇宙结构如恒星和类星体的形成时间表提供了关键证据.
  • 这些早期的物体发射出高能光子,这些光子对于在大爆炸后存在的中性的电离是必不可少的.

研究的目的:

  • 在高红移 (z ≈ 6.3) 时,研究星际介质 (IGM) 中的中性分数.
  • 了解宇宙的再电离历史和早期宇宙物体的作用.

主要方法:

  • 来自已知最遥远的两个类星体的光谱分析.
  • 测量波长短于中性的莱曼α过渡的光子的吸收.

主要成果:

  • 光谱显示了在z ≈ 6.3.3的IGM中的不完全电离.
  • 类星活动前的中性分数明显高于此前估计的 (约0.1%).

结论:

  • 这些发现表明,宇宙的电离历史比以前建模的更为复杂.
  • 在平均电离历史上有潜在的第二个峰值,可能与早期恒星形成和类星体活动有关.