関連する実験動画
Updated: May 31, 2026

11:20
Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
遥か遠くにある銀河の核から発する,非常に明るいパンクロマティックな爆発
A J Levan1, N R Tanvir, S B Cenko
1Department of Physics, University of Warwick, Coventry, UK. a.j.levan@warwick.ac.uk
まとめ
天文学者は,これまで見たことのない,長時間続く高エネルギー放射を持つ,ユニークな,非常に明るい宇宙イベントを観測しました. この強力な爆発は,銀河の中心にある巨大なブラックホールを含む希少なメカニズムから発生した可能性が高い.
科学分野:
- 高エネルギー天体物理学
- 多波長天文学の多波長天文学
- コスミック・トランジエント
背景:
- 変数のX線とガンマ線放射は,極端な宇宙の過程を意味する.
- スウィフト衛星は,ガンマ線で選択されたトランジタを検出します.
研究 の 目的:
- 独特のガンマ線トランジントの多波長観測を提示する.
- その電磁スペクトルと性質を特徴付けるために.
- この前例のない現象の起源を特定するために.
主な方法:
- ガンマ線検出のためにSwift衛星を利用した.
- 電磁スペクトル全体で多波長観測を行った.
- 宿主銀河内のイベントの場所を特定しました.
主要な成果:
- 独特のガンマ線トランジタが検出され,非常に明るく,幅広いスペクトルの放射が検出されました.
- 恒星形成銀河の中心に,赤道偏移 z = 0.3534.4 で発生した.
- 典型的なガンマ線爆発をはるかに上回る長期にわたる高エネルギー放射が観測されました.
- 測定されたピークの明るさは,明るい活発な銀河核のおよそ100倍です.
結論:
- トランジエントの性質は,これまで観測された宇宙源とは異なり,
- 銀河核との関連は,中央の巨大なブラックホールを含む珍しいメカニズムを示唆しています.
関連する概念動画
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...
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...
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...
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.
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...
A pair of electrons in a...
Atomic Emission Spectroscopy: Lab
AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
Atomic Nuclei: Larmor Precession Frequency
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...

