Constraining gravitational wave velocities using gravitational and electromagnetic wave observations of white dwarf binaries
Tian-Yong Cao, Ankit Kumar, and Shu-Xu Yi

TL;DR
This study proposes a method to constrain the difference in propagation speeds of gravitational and electromagnetic waves using white dwarf binary observations, testing fundamental physics beyond general relativity.
Contribution
It introduces a novel approach combining GW and optical data from white dwarf binaries to tightly constrain GW velocity and related fundamental physics parameters.
Findings
Constrained the difference in GW and EM wave speeds to within approximately 10^-12 of the speed of light.
Set upper bounds on the graviton mass at 3×10^-23 eV/c^2.
Limited Lorentz violation parameter within a narrow range.
Abstract
Although the general theory of relativity (GR) predicts that gravitational waves (GWs) have exactly the same propagation velocity as electromagnetic (EM) waves, many theories of gravity beyond GR expect otherwise. Accurate measurement of the difference in their propagation speed, or a tight constraint on it, could be crucial to validate or put limits on theories beyond GR. The proposed future space-borne GW detectors are poised to detect a substantial number of Galactic white dwarf binaries (GWDBs), which emit the GW as semi-monochromatic signals. Concurrently, these GWDBs can also be identified as optical variable sources. Here we proposed that allocating a GWDB's optical light curve and contemporaneous GW signal can be used to trace the difference between the velocity of GW and EM waves. Simulating GW and EM wave data from 14 verification binaries (VBs), our method constrains…
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.
