English

Reducing tilt-to-length coupling for the LISA test mass interferometer

Instrumentation and Methods for Astrophysics 2018-04-24 v1 Optics

Abstract

Objects sensed by laser interferometers are usually not stable in position or orientation. This angular instability can lead to a coupling of angular tilt to apparent longitudinal displacement -- tilt-to-length coupling (TTL). In LISA this is a potential noise source for both the test mass interferometer and the long-arm interferometer. We have experimentally investigated TTL coupling in a setup representative for the LISA test mass interferometer and used this system to characterise two different imaging systems (a two-lens design and a four-lens design) both designed to minimise TTL coupling. We show that both imaging systems meet the LISA requirement of +-25 um/rad for interfering beams with relative angles of up to +-300 urad. Furthermore, we found a dependency of the TTL coupling on beam properties such as the waist size and location, which we characterised both theoretically and experimentally.

Keywords

Cite

@article{arxiv.1711.10320,
  title  = {Reducing tilt-to-length coupling for the LISA test mass interferometer},
  author = {M Tröbs and S Schuster and M Lieser and M Zwetz and M Chwalla and K Danzmann and G Fernandez Barranco and E D Fitzsimons and O Gerberding and G Heinzel and C J Killow and M Perreur-Lloyd and D I Robertson and T S Schwarze and G Wanner and H Ward},
  journal= {arXiv preprint arXiv:1711.10320},
  year   = {2018}
}

Comments

This work will be submitted to CQG

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