相关实验视频
Updated: May 10, 2026

11:20
Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
引力波源GW170817的早期光谱:中子星合并的演变
B J Shappee1,2, J D Simon3, M R Drout3
1The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA. shappee@hawaii.edu.
概括
斯沃普超新星调查2017a (SSS17a) 的光谱显示其快速膨胀和冷却的喷射物. 早期的蓝色成分表明没有化物的物质,而晚期的红色成分与中子星融合喷射模型相匹配.
科学领域:
- 天体物理学
- 多传递器天文学
背景情况:
- 2017年8月17日发现了双中子星合并的光学对应物GW170817 SSS17a.
- 双中子星的合并是理解重元素核合成和引力波源的关键事件.
研究的目的:
- 进行SSS17a的时间序列光谱,以分析喷射物组成和动态.
- 将观测数据与中子星合并喷射的理论模型进行比较.
主要方法:
- 从合并后11.75小时到8.5天的SSS17a的时间序列光谱.
- 黑体适合光谱数据来确定温度和速度.
- 分析光谱特征以确定材料组成.
主要成果:
- 光球在第一个小时内从[公式:见文本]降温到[公式:见文本]K.
- 光球速度大约达到光速的30%.
- Spectra显示出明显的蓝色 (早期) 和红色 (晚期) 成分,在几天内演变.
结论:
- 晚期的光谱成分与R-过程丰富的中子星喷射物保持一致.
- 早期的蓝色成分表明存在高速度,无化物材料.
- 这些发现为中子星的融合和重元素的形成提供了关键的见解.
相关概念视频
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 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...
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 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...
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: 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,...
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...

