相关实验视频
Updated: Jul 19, 2026

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High Resolution Phonon-assisted Quasi-resonance Fluorescence Spectroscopy
Published on: June 28, 2016
对于GRB 990123的距离和能量释放的光谱极限
Andersen1, Castro-Tirado, Hjorth
1Nordic Optical Telescope, Apartado 474 St. Cruz de La Palma, E-38700 Canarias, Spain. Laboratorio de Astrofisica Espacial y Fisica Fundamental, Instituto Nacional de Tecnica Aeroespacial, Post Office Box 50727, E-28080 Madrid, Spain. Insti.
概括
这项研究确定了明亮的马射线爆发GRB 990123.3的特定红移 (z=1.600). 这一发现有助于解释宇宙事件释放的巨大能量.
科学领域:
- 天文学和天体物理学
- 宇宙事件 宇宙事件
- 频谱学是一种光谱学.
背景情况:
- 马射线爆发 (GRBs) 是宇宙中最明亮的事件.
- 了解GRB的红移和能量输出对于宇宙学至关重要.
- GRB 990123是一个非常明亮的事件,促使详细的调查.
研究的目的:
- 为了确定马射线爆发GRB 990123.3的红移.
- 为了限制GRB 990123.3的能量释放.
- 调查对宇宙学模型的影响.
主要方法:
- 在GRB 990123的光学光谱学后发光.
- 分析频谱中的吸收系统.
- 紫外线光度测定用于设置红移的上限.
主要成果:
- 在z = 1.600的红移处检测到一个吸收系统.
- 红移的上限被确定为z < 2.17 (莱曼α森林) 和z < 2.05 (UV光度).
- 观察到的吸收系统强烈表明GRB 990123发生在z = 1.600.
结论:
- 对于GRB 990123而言,z = 1.600的红移是统计学上显著的.
- 巨大的能量释放 (4.5 x 10^54 erg) 挑战了当前的宇宙学参数.
- 非同位素排放模型,如内在辐射,可以解决能量差异.
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