使用与卡西尼号航天器的无线电连接进行广义相对论的测试
B Bertotti1, L Iess, P Tortora
1Dipartimento di Fisica Nucleare e Teorica, Università di Pavia, Via U. Bassi 6, I-27100, Pavia, Italy.
Nature
|September 26, 2003
概括
这项研究测量了靠近太阳的无线电光子的频率转移,证实了爱因斯坦的广义相对论. 精确的测量接近在某些宇宙学模型中理论上预测的偏差水平.
科学领域:
- 物理 物理学 物理
- 天文学 天文学
- 宇宙学的宇宙学是什么?
背景情况:
- 一般相对论预测光子偏移和延迟是由于质量引起的时空曲率造成的.
- 参数gamma量化了牛顿引力偏差,在广义相对论中的统一性.
- 以前的实验证实了广义相对论的预测,准确度为~0.1%.
研究的目的:
- 测量通过太阳附近的无线电光子的频率转移.
- 以高精度测试广义相对论的预测.
- 探测一些宇宙学模型预测的微小,可检测的效应.
主要方法:
- 利用无线电光子从卡西尼航天器到卡西尼航天器旅行.
- 测量了光子经过太阳附近时的频率变化.
- 分析数据以确定参数gamma的值.
主要成果:
- 测量到的马值为1 + (2.1 ± 2.3) x 10^-5. 这样,马的测量值是1 + (2.1 ± 2.3) x 10^-5.
- 这一结果与标准广义相对论的预测一致.
- 测量的灵敏度接近用于检测偏差的理论值.
结论:
- 这项研究为广义相对论提供了强有力的实验支持.
- 这些发现限制了预测偏离广义相对论的理论.
- 未来的研究可以更精确地探索微妙的宇宙学效应.
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