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一个带有引力透镜的类星体,其四个图像分别为14.62弧秒
Naohisa Inada1, Masamune Oguri, Bartosz Pindor
1Department of Physics, School of Science, The University of Tokyo, 113-0033, Japan. inada@utap.phys.s.u-tokyo.ac.jp
Nature
|December 20, 2003
概括
天文学家发现了一个带有引力透镜的类星体,SDSS J1004+4112,其距离是创纪录的14.62弧秒. 这一发现支持冷暗物质模型,表明透镜物体主要由暗物质主导.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 暗物质研究 暗物质研究
背景情况:
- 引力透镜对于绘制暗物质分布的地图至关重要.
- 冷暗物质模型预测大分离透镜类星体,但很少有人发现.
- 现有的透镜类星体有很小的分离,归因于微粒子物质.
研究的目的:
- 为了寻找和报告发现一个大分离的引力透镜类星体.
- 提供支持冷暗物质模型的观测证据.
- 为了利用类星体作为宇宙学探测器,由于更简单的镜头系统.
主要方法:
- 寻找表现出引力透镜效应的类星体.
- 分析了透镜类星体组件的图像分离.
- 在冷暗物质模型框架内解释结果.
主要成果:
- 发现了一个重力透镜类星体,SDSS J1004+4112.
- 测量了最大的组件分离14.62弧秒.
- 很大的分离强烈地表明透镜质量是由暗物质主导的.
结论:
- 发现SDSS J1004+4112与冷暗物质模型的预测一致.
- 这一发现验证了模型对大规模结构形成的预测.
- 大分离透镜类星体是研究暗物质的宝贵工具.
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