A New Method to Test the Einstein's Weak Equivalence Principle
H. Yu, S. Q. Xi, F. Y. Wang (NJU)

TL;DR
This paper introduces a novel method to test Einstein's Weak Equivalence Principle by utilizing the direction-dependent gravitational time delay, allowing for more accurate constraints on potential violations compared to previous methods.
Contribution
The authors propose a new approach that naturally corrects for confounding effects in gravitational time delay measurements, improving the precision of WEP tests.
Findings
Constraint on $\Delta \gamma$ as low as 10^{-14}
Method effectively isolates gravitational time delay from other effects
Potential for tighter constraints with future observations
Abstract
The Einstein's weak equivalence principle (WEP) is one of the foundational assumptions of general relativity and some other gravity theories. In the theory of parametrized post-Newtonian (PPN), the difference between the PPN parameters of different particles or the same type of particle with different energies, , represents the violation of WEP. Current constraints on are derived from the observed time delay between correlated particles of astronomical sources. However, the observed time delay is contaminated by other effects, such as the time delays due to different particle emission times, the potential Lorentz invariance violation and none-zero photon rest mass. Therefore, current constraints are only upper limits. Here we propose a new method to test WEP based on the fact that the gravitational time delay is direction-dependent while others…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
