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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
来自遥远宇宙中的分子的可变质子对电子质量比的强限
Michael T Murphy1, Victor V Flambaum, Sébastien Muller
1Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H39, Post Office Box 218, Victoria 3122, Australia. mmurphy@swin.edu.au
概括
科学家们使用来自类星体的氨光谱测试了质子对电子质量比 (mu). 这项研究为mu的变化提供了迄今为止最强大的天体物理约束,表明它在宇宙时间上是恒定的.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
背景情况:
- 粒子物理学的标准模型假定基本常数是不变的.
- 宇宙观测,例如类星体吸收线,可以在巨大的距离和时间尺度上测试这些常数.
- 质子与电子的质量比 (mu) 是一个对变化敏感的关键基本常数.
研究的目的:
- 用分子光谱学测量质子对电子的质量比 (mu).
- 通过使用类星体视线来限制宇宙时间内mu的潜在变化.
主要方法:
- 利用氨逆转过渡,这是高度敏感的.
- 从类星体B0218+357获得的高质量的氨光谱与实验室旋转光谱进行了比较.
- 分析了沿着类星体视线的分子云中的吸收线,以探测 mu.
主要成果:
- 介绍了使用这种光谱技术的第一个详细测量mu.
- 在95%的信心下,从Mu的实验室值到Deltamu/mu干 <1.8 x 10(-6) 的受约束的相对偏差.
- 在大约宇宙当前年龄的一半的mu上实现了迄今为止最强的天体物理约束.
结论:
- 质子与电子的质量比 (mu) 在整个宇宙时间表中显示出了显著的稳定性.
- 氨光谱是测试基本物理常数的强大工具.
- 未来高质量的氨观测可以进一步减少mu测量的不确定性.
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