
TL;DR
This paper introduces Geometric TDI, a new approach to analyze and optimize Time Delay Interferometry observables for LISA, enhancing sensitivity and robustness against noise and instrumental issues.
Contribution
It presents a combinatorial algorithm for exploring second-generation TDI observables, identifying improved forms with better sensitivity and noise resilience.
Findings
Identified alternative TDI observables with fewer nulls in response functions.
Discovered TDI forms less susceptible to instrumental gaps and glitches.
Enhanced high-frequency gravitational-wave sensitivity.
Abstract
The space-based gravitational-wave observatory LISA, a NASA-ESA mission to be launched after 2012, will achieve its optimal sensitivity using Time Delay Interferometry (TDI), a LISA-specific technique needed to cancel the otherwise overwhelming laser noise in the inter-spacecraft phase measurements. The TDI observables of the Michelson and Sagnac types have been interpreted physically as the virtual measurements of a synthesized interferometer. In this paper, I present Geometric TDI, a new and intuitive approach to extend this interpretation to all TDI observables. Unlike the standard algebraic formalism, Geometric TDI provides a combinatorial algorithm to explore exhaustively the space of second-generation TDI observables (i.e., those that cancel laser noise in LISA-like interferometers with time-dependent armlengths). Using this algorithm, I survey the space of second-generation TDI…
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.
