Time-Delay Interferometry
Massimo Tinto, and Sanjeev V. Dhurandhar

TL;DR
Time-Delay Interferometry (TDI) is a technique designed to cancel laser noise in space-based gravitational wave detectors with unequal arm lengths, enabling precise phase measurements crucial for missions like LISA.
Contribution
This paper provides a comprehensive overview of the theoretical foundations and mathematical principles of TDI for space-based interferometers.
Findings
Explains how TDI cancels laser noise in unequal arm interferometers.
Details the mathematical framework for implementing TDI in space missions.
Prepares for future practical and experimental developments in TDI.
Abstract
Equal-arm interferometric detectors of gravitational radiation allow phase measurements many orders of magnitude below the intrinsic phase stability of the laser injecting light into their arms. This is because the noise in the laser light is common to both arms, experiencing exactly the same delay, and thus cancels when it is differenced at the photo detector. In this situation, much lower level secondary noises then set overall performance. If, however, the two arms have different lengths (as will necessarily be the case with space-borne interferometers), the laser noise experiences different delays in the two arms and will hence not directly cancel at the detector. In order to solve this problem, a technique involving heterodyne interferometry with unequal arm lengths and independent phase-difference readouts has been proposed. It relies on properly time-shifting and linearly…
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.
