Laser-Frequency Stabilization via a Quasimonolithic Mach-Zehnder Interferometer with Arms of Unequal Length and Balanced dc Readout
Oliver Gerberding, Katharina-Sophie Isleif, Moritz Mehmet and, Karsten Danzmann, Gerhard Heinzel

TL;DR
This paper presents a simple, low-noise laser frequency stabilization method using a quasimonolithic Mach-Zehnder interferometer with unequal arms and balanced detection, achieving high stability suitable for gravitational wave detection.
Contribution
The authors demonstrate a novel laser stabilization scheme with minimal optical components, no additional modulations, and low frequency noise, meeting stringent space-based interferometry requirements.
Findings
Frequency noise below 100 Hz/√Hz at 1 Hz
Achieved LISA pre-stabilization requirement of 300 Hz/√Hz down to 100 mHz
Designed interferometer minimizes thermal and stray light effects
Abstract
Low frequency high precision laser interferometry is subject to excess laser-frequency-noise coupling via arm-length differences which is commonly mitigated by locking the frequency to a stable reference system. This approach is crucial to achieve picometer level sensitivities in the 0.1 mHz to 1 Hz regime, where laser frequency noise is usually high and couples into the measurement phase via arm-length mismatches in the interferometers. Here we describe the results achieved by frequency stabilising an external cavity diode laser to a quasi-monolithic unequal arm-length Mach-Zehnder interferometer read out at mid-fringe via balanced detection. We find this stabilization scheme to be an elegant solution combining a minimal number of optical components, no additional laser modulations and relatively low frequency noise levels. The Mach-Zehnder interferometer has been designed and…
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