一个宇宙起源的静态引力波背景的上限
1, B P Abbott, R Abbott
1Lists of participants and their affiliations appear at the end of the paper.
Nature
|August 21, 2009
概括
科学家使用LIGO数据为静态引力波背景设定了新的极限. 这项研究探讨了早期的宇宙,为宇宙进化提供了洞察力,并排除了某些宇宙学模型.
科学领域:
- 宇宙学和天体物理学
- 引力波天文学 引力波天文学
- 早期宇宙物理学 早期宇宙物理学
背景情况:
- 从许多未解决的天体物理学和宇宙学来源预测引力波的随机背景.
- 这个背景包含来自宇宙最早时刻的独特签名,对于理解宇宙进化至关重要.
- 对这种背景的直接测量对于研究宇宙在一分钟之前的年龄至关重要.
研究的目的:
- 为了确定静态引力波背景振幅的极限.
- 为了利用激光干扰仪引力波天文台 (LIGO) 的数据进行这项调查.
- 限制早期宇宙进化模型和宇宙弦理论的模型.
主要方法:
- 来自激光干扰仪引力波观测台 (LIGO) 的两年科学运行数据的分析.
- 设定静态引力波背景能量密度的上限.
- 专注于100赫兹左右的频段.
主要成果:
- 限制了随机引力波背景的正常化能量密度在95%的信心下小于6.9 x 10^-6.
- 排除了具有较大的状态方程参数的早期宇宙进化模型.
- 排除了一些弦理论模型中偏爱的具有小弦张力的宇宙 (超级) 弦模型.
结论:
- 该研究提供了迄今为止对100 Hz的随机引力波背景的最严格的限制.
- 这些结果改善了从大爆炸核合成和宇宙微波背景辐射中获得的间接极限.
- 这些发现对测试早期宇宙的基本物理学有重大意义.
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