Influence of EOM sideband modulation noise on space-borne gravitational wave detection
Mingyang Xu, Yujie Tan, Hanzhong Wu, Panpan Wang, Hao Yan, and Yurong Liang, Chenggang Shao

TL;DR
This paper analyzes the impact of EOM sideband modulation noise on space-borne gravitational wave detection, deriving strict noise requirements and experimentally verifying a commercial EOM's suitability for LISA.
Contribution
It provides a rigorous analytic expression for modulation noise requirements and experimentally confirms a commercial EOM's capability to meet these standards for GW detection.
Findings
Derived strict modulation noise requirement expression.
Experimental verification of commercial EOM meeting LISA's noise standards.
EOM can support future improved displacement measurement accuracy.
Abstract
Clock noise is one of the dominant noises in the space-borne gravitational wave (GW) detection. To suppress this noise, the clock noise-calibrated time-delay-interferometry (TDI) technique is proposed. In this technique, an inter-spacecraft clock tone transfer chain is necessary to obtain the comparison information of the clock noises in two spacecraft, during which an electro-optic-modulator (EOM) is critical and used to modulate the clock noise to the laser phase. Since the EOM sideband modulation process introduces modulation noise, it is significant to put forward the corresponding requirements and assess whether the commercial EOM meets. In this work, based on the typical Michelson TDI algorithm and the fundamental noise requirement of GW detectors, the analytic expression of the modulation noise requirement is strictly derived, which relax the component indicator need compared to…
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Taxonomy
TopicsAdvanced Frequency and Time Standards · Pulsars and Gravitational Waves Research · Advanced Fiber Laser Technologies
