Testing the nature of gravitational-wave polarizations using strongly lensed signals
Srashti Goyal, K. Haris, Ajit Kumar Mehta, Parameswaran Ajith

TL;DR
This paper explores how strong gravitational lensing of gravitational waves can enhance the ability of detector networks to test the fundamental polarization modes predicted by general relativity and alternative theories.
Contribution
It demonstrates that observing multiple lensed copies of the same GW signal effectively increases detector count, improving polarization mode discrimination.
Findings
Lensed GW signals improve polarization mode testing.
Multiple images enable better model distinction.
Enhanced detection sensitivity for alternative gravity theories.
Abstract
Gravitational-wave (GW) observations by a network of ground-based laser interferometric detectors allow us to probe the nature of GW polarizations. This would be an interesting test of general relativity (GR), since GR predicts only two polarization modes while there are theories of gravity that predict up to six polarization modes. The ability of GW observations to probe the nature of polarizations is limited by the available number of linearly independent detectors in the network. (To extract all polarization modes, there should be at least as many detectors as the polarization modes.) Strong gravitational lensing of GWs offers a possibility to significantly increase the effective number of detectors in the network. Due to strong lensing (e.g., by galaxies), multiple copies of the same signal can be observed with time delays of several minutes to weeks. Owing to the rotation of the…
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.
