Renzhi Su, 仁智 苏, Tao An, Stephen J. Curran, Michael P. Busch, Minfeng Gu and Di Li
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引用次数: 0
摘要
引力的量子性质仍然是现代物理学最大的谜团之一,许多统一理论都预测了基本常数在不同时空的变化。在这里,我们展示了在星系动力学时间尺度上对这些变化的精确测量--这是一个关键但以前从未探索过的机制。通过同时观测 M31 中的 H i 和 OH 线,我们探测了 250 万年回溯时间内基本常数的潜在变化。我们得到了Δ(μα2)/(μα2) < 4.6 × 10-3,Δgp/gp < 7.2 × 10-3,其中α是精细结构常数,μ是质子-电子质量比,gp是质子g因子。这些结果弥合了实验室测试与宇宙学观测之间的差距,对局部动力学与基础物理学之间的耦合提供了独特的见解。我们的发现对预测银河系时间尺度上的显著变化的理论提出了挑战,同时展示了量子引力模型的一个强大的新探针。
Constraints on the Fractional Changes of the Fundamental Constants at a Look-back Time of 2.5 Myr
The quantum nature of gravity remains one of the greatest mysteries of modern physics, with many unified theories predicting variations in fundamental constants across space and time. Here we present precise measurements of these variations at galactic dynamical timescales—a critical but previously unexplored regime. Using simultaneous observations of H i and OH lines in M31, we probe potential variations of fundamental constants at a look-back time of 2.5 million yr. We obtained , with complementary constraints on Δ(μα2)/(μα2) < 4.6 × 10−3, and Δgp/gp < 7.2 × 10−3, where α is the fine structure constant, μ is the proton–electron mass ratio, and gp is the proton g-factor. These results bridge the gap between laboratory tests and cosmological observations, providing unique insights into the coupling between local dynamics and fundamental physics. Our findings challenge theories predicting significant variations over galactic timescales while demonstrating a powerful new probe of quantum gravity models.