Testing general relativity

Image credit: [InformiguelCarreño (Own work) [CC BY-SA 4.0], via Wikimedia Commons]

Einstein’s general relativity is the basis of modern astronomy and astrophysics. Therefore, testing the validity of basic assumptions made in general relativity is significant. One of the basic assumptions of general relativity is the so-called ‘Einstein’s weak equivalence principle (WEP)’. WEP means that speeds of lights with different frequencies are exactly the same in a vacuum. If WEP is violated, the speeds of lights would be slightly different for different frequencies, resulting in an arrival time lag between different frequencies. How can we accurately measure such a time lag?

I propose a new method to accurately measure the time lag between different frequencies using fast radio bursts (FRBs). FRBs are millisecond pulses in radio coming from distant galaxies. The long distances to FRBs and their short timescales provide an ideal laboratory to strongly constrain the hypothetical time lag.

If WEP is violated (i.e., the speeds of lights are different for different frequencies in a vacuum), such violation has to be within the observational uncertainty of FRB’s arrival time. This is because we do not see any significant time lag of the FRB emission using current radio telescopes after removing a plasma effect that causes an additional time lag. Therefore, we propose to use the observational uncertainty of FRB’s arrival time to strongly constrain the WEP violation.

Figure: Upper limits on log Δγ placed by FRBs (red dots: this work) and previous works (black markers). The smaller log Δγ indicates the tighter constraint. I achieved three orders of magnitude tighter constraint on the WEP violation than previous works.
Figure: Upper limits on log Δγ placed by FRBs (red dots: this work) and previous works (black markers). The smaller log Δγ indicates the tighter constraint. I achieved three orders of magnitude tighter constraint on the WEP violation than previous works.
The figure shows the upper limits on log Δγ that is an indicator of how accurately WEP is confirmed. The smaller log Δγ indicates the tighter constraint on the WEP violation. I achieved three orders of magnitude tighter constraint (red dots) than previous works (black markers) using my unique method and FRBs. General relativity is found to be correct up to 10^-21 accuracy! In the future, we may be able to see something beyond general relativity using FRBs.

This project is based on the following publication.

Tetsuya Hashimoto, Tomotsugu Goto, Daryl Joe D. Santos, Simon C.-C. Ho, Ece Kilerci-Eser, Tiger Y.-Y. Hsiao, Yi Hang Valerie Wong, Alvina Y. L. On, Seong Jin Kim, and Ting-Yi Lu, 'Upper limits on Einstein's weak equivalence principle placed by uncertainties of dispersion measures of fast radio bursts' , accepted for publication in accepted for publication in Physical Review D, (2021).

Please see also

Kaustubha Sen, Tetsuya Hashimoto, Tomotsugu Goto, Seong Jin Kim, Bo Han Chen, Daryl Joe D. Santos, Simon C. C. Ho, Alvina Y. L. On, Ting-Yi Lu, and Tiger Y.-Y. Hsiao, 'Constraining violations of the Weak Equivalence Principle Using CHIME FRBs' , accepted for publication in Monthly Notices of the Royal Astronomical Society, (2021).

This paper was featured by ‘Medium’, 'Testing Einstein’s Work Using Observations of Fast Radio Bursts' .

Tetsuya Hashimoto
Tetsuya Hashimoto
Assistant professor (NCHU)