用银河系红移扭曲来测试宇宙加速的性质
L Guzzo1, M Pierleoni, B Meneux
1INAF-Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate, LC, Italy. luigi.guzzo@brera.inaf.it
Nature
|February 1, 2008
概括
科学家测量了0.8红移时宇宙结构的增长,发现结果与标准暗能模型一致. 需要进一步的观察来区分暗能量理论.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 一般相对论一般相对论.
背景情况:
- 宇宙的加速膨胀归因于暗能量,暗能量是一个神秘的组成部分,占宇宙能量密度的75%左右.
- 宇宙常数是最简单的暗能量候选者,但其他选择包括标量场或改性引力.
- 不同的暗能量模型预测大规模结构的不同增长率.
研究的目的:
- 测量宇宙结构在红移z=0.8.8时的增长速度.
- 通过分析星系运动来测试不同暗能量模型的预测.
主要方法:
- 利用了一项新的银河系红移调查,对1万多个昏暗的星系进行了调查.
- 测量了星系聚类中的辐射异型性,这是结构增长的指纹.
- 计算了异构性参数β和结构生长率f.
主要成果:
- 测量的异性异性参数β = 0.70 ± 0.26.
- 计算的结构增长率 f = 0.91 ± 0.36 在红移 0.8.8 时.
- 结果与具有低物质密度和平面几何形状的标准宇宙学常量模型一致.
结论:
- 目前的测量支持标准暗能模型,但还不能排除其他理论.
- 需要进行更大规模的调查,将采样量增加十倍,以区分暗能量模型.
- 这项研究为暗能量和宇宙膨胀的性质提供了关键的观测约束.
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