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Average Acceleration01:30

Average Acceleration

9.6K
The importance of understanding acceleration spans our day-to-day experiences, as well as the vast reaches of outer space and the tiny world of subatomic physics. In everyday conversation, to accelerate means to speed up. For instance, we are familiar with the acceleration of our car; the harder we apply our foot to the gas pedal, the faster we accelerate. The greater the acceleration, the greater the change in velocity over a given time. Acceleration is widely seen in experimental physics. In...
9.6K
Nuclear Transmutation03:20

Nuclear Transmutation

17.6K
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...
17.6K
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

2.0K
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.
2.0K
Detection of Black Holes01:10

Detection of Black Holes

2.2K
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...
2.2K
Mass Analyzers: Common Types01:19

Mass Analyzers: Common Types

612
The quadrupole mass analyzer consists of four cylindrical metal rods arranged in a diamond carrying a DC voltage and a radio-frequency AC voltage. The motion of ions through the quadrupole depends on the field strength, causing only ions of a certain m/z to resonate successfully and strike the detector at a given field strength. Though the transmission rate for these analyzers is high, the exact elemental composition of the sample is not determined because of low resolution; however, they are...
612
Motion Of A Charged Particle In A Magnetic Field01:22

Motion Of A Charged Particle In A Magnetic Field

4.8K
A charged particle experiences a force when moving through a magnetic field. Consider the field to be uniform and the charged particle to move perpendicular to it. If the field is in a vacuum, the magnetic field is the dominant factor determining the motion. Since the magnetic force is perpendicular to the direction of motion, a charged particle follows a curved path. The particle continues to follow this curved path until it forms a complete circle. Another way to look at this is that the...
4.8K

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A galactic microquasar mimicking winged radio galaxies.

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関連する実験動画

Updated: Jul 5, 2025

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

12.8K

銀河の粒子加速器で

Valentí Bosch-Ramon1

  • 1Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos Universitat de Barcelona (ICCUB), Universitat de Barcelona (IEEC-UB), E08028 Barcelona, Catalonia, Spain.

Science (New York, N.Y.)
|January 25, 2024
PubMed
まとめ

私たちの銀河系で最も強力なプラズマジェットは 非常に高エネルギーのガンマ線を放出します これらの宇宙現象は 高エネルギー天体物理学を理解するための鍵です

科学分野:

  • 天体物理学
  • 高エネルギー物理学

背景:

  • プラズマジェットは 強い電離物質の流れです
  • 銀河系には最もエネルギーに満ちた 天体物理現象がいくつかあります

研究 の 目的:

  • 銀河の強力なプラズマジェットの 放射特性を調べるために
  • このジェットで発生する 高エネルギーガンマ線の性質を 特定するためです

主な方法:

  • ガンマ線望遠鏡を用いた観測天文学
  • ガンマ線放射のスペクトルおよび時間特性の分析.

主要な成果:

  • 強力なプラズマジェットからの 高エネルギーガンマ線の検出
  • ジェット活動とガンマ線光の相関

結論:

  • 強力なプラズマジェットは 非常に高エネルギーガンマ線の 確認された源です
  • これらの発見は 極端な天体物理的過程と 粒子加速の理解を 進めているのです

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