Design method for the structure of a gravitational wave detection telescope with low TTL noise

Design method for the structure of a gravitational wave detection telescope with low TTL noise

Abstract As a critical payload of the gravitational wave detection interferometry system, the tilt-to-length (TTL) noise has a significant influence on the detection accuracy of the interferometry system. The non-geometric TTL (NG-TTL) noise, which is the main component of the TTL noise within the t...

Full description

Saved in:
Bibliographic Details
Main Authors: Sijun Fang, Wentong Fan, Rui Zhang, Jian Luo, Bohong Li, Hongwen Hai, Yehao Cao, Lei Fan, Yong Yan
Format: Article
Language:English
Published: Nature Portfolio 2024-11-01
Series:Scientific Reports
Subjects:
Tilt-to-length noise
Sensitive aberrations
Structural deformations of the telescope
Desensitization design method
Online Access:https://doi.org/10.1038/s41598-024-80692-9
Tags: Add Tag
No Tags, Be the first to tag this record!

Internet

https://doi.org/10.1038/s41598-024-80692-9

Similar Items