# New test of weak equivalence principle using polarized light from   astrophysical events

**Authors:** Xue-Feng Wu, Jun-Jie Wei, Mi-Xiang Lan, He Gao, Zi-Gao Dai, Peter, M\'esz\'aros

arXiv: 1703.09935 · 2017-05-05

## TL;DR

This paper tests Einstein's weak equivalence principle using polarized light from astrophysical events, setting new stringent limits on deviations across multiple wavelengths and confirming the principle's validity with unprecedented precision.

## Contribution

It introduces a novel method to constrain the WEP using polarized photons from astrophysical transients, achieving the most stringent limits to date across different bands.

## Key findings

- Set upper limits on $	riangle	ext{γ}$ for polarized photons from GRBs and FRBs.
- First direct verification of WEP for multiband polarized photons.
- Improved the previous best WEP deviation limit by an order of magnitude.

## Abstract

Einstein's weak equivalence principle (WEP) states that any freely falling, uncharged test particle follows the same identical trajectory independent of its internal structure and composition. Since the polarization of a photon is considered to be part of its internal structure, we propose that polarized photons from astrophysical transients, such as gamma-ray bursts (GRBs) and fast radio bursts (FRBs), can be used to constrain the accuracy of the WEP through the Shapiro time delay effect. Assuming that the arrival time delays of photons with different polarizations are mainly attributed to the gravitational potential of the Laniakea supercluster of galaxies, we show that a strict upper limit on the differences of the parametrized post-Newtonian parameter $\gamma$ value for the polarized optical emission of GRB 120308A is $\Delta\gamma<1.2\times10^{-10}$, for the polarized gamma-ray emission of GRB 100826A is $\Delta\gamma<1.2\times10^{-10}$, and for the polarized radio emission of FRB 150807 is $\Delta\gamma<2.2\times10^{-16}$. These are the first direct verifications of the WEP for multiband photons with different polarizations. In particular, the result from FRB 150807 provides the most stringent limit to date on a deviation from the WEP, improving by one order of magnitude the previous best result based on Crab pulsar photons with different energies.

## Full text

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## References

46 references — full list in the complete paper: https://tomesphere.com/paper/1703.09935/full.md

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Source: https://tomesphere.com/paper/1703.09935