Speaker
Yujie Tan
(Huazhong University of Science and Technology)
Description
Space-based gravitational wave detection (e.g., LISA, Taiji, and TianQin) relies on ultra-high-precision inter-satellite laser interferometry. However, clock noise is approximately two orders of magnitude higher than the detector noise floor, which severely limits the overall detection sensitivity and becomes a critical constraint for space-based gravitational wave observatories. To address this challenge, this presentation reports our recent progress in both theoretical and experimental studies on clock noise suppression.
Primary author
Yujie Tan
(Huazhong University of Science and Technology)
