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从局部快速无线电爆发中对宇宙中的子进行普查
J-P Macquart1, J X Prochaska2,3, M McQuinn4
1International Centre for Radio Astronomy Research, Curtin Institute of Radio Astronomy, Curtin University, Perth, Western Australia, Australia. J.Macquart@curtin.edu.au.
研究人员使用快速无线电爆发 (FRB) 测量了宇宙的 baryons 含量. 这种新方法准确地计算了离子化子, 提供了与其他宇宙测量一致的宇宙密度.
科学领域:
- 宇宙学
- 天体物理学
- 宇宙微波背景
背景情况:
- 大多数宇宙的重子物质是分散的, 很难检测.
- 像类星光谱和X射线辐射研究这样的先前方法在灵敏度和范围上有局限性.
- 现有的技术难以准确地测量宇宙体积中的"隐形"重子.
研究的目的:
- 为了独立测量宇宙子密度.
- 开发一种新技术来检测扩散的微子物质.
- 使用快速无线电爆发分散来计算所有电离化的子.
主要方法:
- 使用局部快速无线电爆发 (FRB) 的散射测量.
- 在FRB视线上确定电子柱密度.
- 在已知红移的宿主星系中增加了现有的FRB样本.
主要成果:
- 导出一个宇宙 baryons 密度的 [公式:见文本].
- 实现了与宇宙微波背景和大爆炸核合成值一致的测量.
- 完成了足够大的FRB样本以考虑分散变化.
结论:
- 快速无线电爆发分散提供了一种可靠的方法来测量宇宙 baryons 密度.
- 这种独立的测量证实了现有的宇宙模型.
- 这项研究成功地描述了宇宙中电离化的子的分布.
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