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関連する概念動画

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...
Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...

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関連する実験動画

Updated: Jul 5, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

銀河間媒質の構造形成からの宇宙ガンマ線背景.

Loeb1, Waxman

  • 1Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA. aloeb@cfa.harvard.edu

Nature
|May 23, 2000
PubMed
まとめ

宇宙構造の形成は相対性電子を生成し,宇宙マイクロ波背景フォトンを散らばし,拡散ガンマ線背景を説明する. この発見は,宇宙学的モデルとビッグバン核合成の予測と一致しています.

科学分野:

  • コスモロジー・コスモロジーとは
  • 天体物理学 天体物理学
  • 高エネルギー天体物理学

背景:

  • 拡散ガンマ線背景の起源は,宇宙学の主要な未解決問題である.
  • 活発な銀河核のような離散的な源は,観測されたガンマ線流の25%未満を占めています.

研究 の 目的:

  • 拡散ガンマ線背景放射の起源を説明するために.
  • 大規模構造形成とガンマ線放射を結びつけるため.

主な方法:

  • 宇宙構造形成中の銀河間媒体の衝撃波のモデリング.
  • 宇宙マイクロ波背景フォトンの放散を,これらの衝撃によって生成された相対性電子によってシミュレートする.

主要な成果:

  • 銀河間媒体の衝撃波は,極めて相対的な電子を生成する.
  • これらの電子は,宇宙マイクロ波の背景フォトンをガンマ線エネルギーに分散させ,拡散した背景を生成します.
  • モデルの予測されたフクロスは,光子のエネルギーにおける四次元の観測値と一致します.

結論:

  • 拡散したガンマ線背景は,宇宙構造形成プロセスによって局所的に生成されます.

さらに関連する動画

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
06:28

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

関連する実験動画

Last Updated: Jul 5, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
06:28

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

  • このモデルは,ガンマ線背景が1度以上の角度スケールで5%以内で同otropicであることを予測しています.
  • この合意は,ビッグバン核合成と一致する平均宇宙学的バリオン密度を暗示している.