pith. sign in

arxiv: gr-qc/0306057 · v1 · submitted 2003-06-13 · 🌀 gr-qc

Time Delay Interferometry and LISA Optimal Sensitivity

classification 🌀 gr-qc
keywords noisedatalaseroptimalsensitivityfrequencylisatime
0
0 comments X
read the original abstract

The sensitivity of LISA depends on the suppression of several noise sources; dominant one is laser frequency noise. It has been shown that the six Doppler data streams obtained from three space-crafts can be appropriately time delayed and optimally combined to cancel this laser frequency noise. We show that the optimal data combinations when operated in a network mode improves the sensitivity over Michelson ranging from 40 % to 100 %. In this article, we summarize these results. We further show that the residual laser noise in the optimal data combination due to typical arm-length inaccuracy of 200 m is much below the level of optical path and the proof mass noises.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.