2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer

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Authors

  • Victor Huarcaya
  • Miguel Dovale Álvarez
  • Daniel Penkert
  • Stefano Gozzo
  • Pablo Martínez Cano
  • Kohei Yamamoto
  • Juan José Esteban Delgado
  • Moritz Mehmet
  • Karsten Danzmann
  • Gerhard Heinzel
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Details

Original languageEnglish
Article number024078
JournalPhysical review applied
Volume20
Issue number2
Publication statusPublished - Aug 2023

Abstract

To achieve subpicometer sensitivities in the millihertz band, laser interferometric inertial sensors rely on some form of reduction of the laser-frequency noise, typically by locking the laser to a stable frequency reference, such as the narrow-line-width resonance of an ultrastable optical cavity or an atomic or molecular transition. In this paper, we report on a compact laser-frequency stabilization technique based on an unequal-arm Mach-Zehnder interferometer that is subnanometer stable at 10μHz, subpicometer at 0.5 mHz, and reaches a noise floor of 7fm/Hz at 1 Hz. The interferometer is used in conjunction with a dc servo to stabilize the frequency of a laser down to a fractional instability below 4×10-13 at averaging times from 0.1 to 100 s. The technique offers a wide operating range, does not rely on complex lock-acquisition procedures, and can be readily integrated as part of the optical bench in future gravity missions.

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Cite this

2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer. / Huarcaya, Victor; Álvarez, Miguel Dovale; Penkert, Daniel et al.
In: Physical review applied, Vol. 20, No. 2, 024078, 08.2023.

Research output: Contribution to journalArticleResearchpeer review

Huarcaya, V, Álvarez, MD, Penkert, D, Gozzo, S, Cano, PM, Yamamoto, K, Delgado, JJE, Mehmet, M, Danzmann, K & Heinzel, G 2023, '2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer', Physical review applied, vol. 20, no. 2, 024078. https://doi.org/10.1103/PhysRevApplied.20.024078
Huarcaya, V., Álvarez, M. D., Penkert, D., Gozzo, S., Cano, P. M., Yamamoto, K., Delgado, J. J. E., Mehmet, M., Danzmann, K., & Heinzel, G. (2023). 2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer. Physical review applied, 20(2), Article 024078. https://doi.org/10.1103/PhysRevApplied.20.024078
Huarcaya V, Álvarez MD, Penkert D, Gozzo S, Cano PM, Yamamoto K et al. 2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer. Physical review applied. 2023 Aug;20(2):024078. doi: 10.1103/PhysRevApplied.20.024078
Huarcaya, Victor ; Álvarez, Miguel Dovale ; Penkert, Daniel et al. / 2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer. In: Physical review applied. 2023 ; Vol. 20, No. 2.
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title = "2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer",
abstract = "To achieve subpicometer sensitivities in the millihertz band, laser interferometric inertial sensors rely on some form of reduction of the laser-frequency noise, typically by locking the laser to a stable frequency reference, such as the narrow-line-width resonance of an ultrastable optical cavity or an atomic or molecular transition. In this paper, we report on a compact laser-frequency stabilization technique based on an unequal-arm Mach-Zehnder interferometer that is subnanometer stable at 10μHz, subpicometer at 0.5 mHz, and reaches a noise floor of 7fm/Hz at 1 Hz. The interferometer is used in conjunction with a dc servo to stabilize the frequency of a laser down to a fractional instability below 4×10-13 at averaging times from 0.1 to 100 s. The technique offers a wide operating range, does not rely on complex lock-acquisition procedures, and can be readily integrated as part of the optical bench in future gravity missions.",
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note = "Funding Information: We would like to thank Germ{\'a}n Fern{\'a}ndez Barranco for his help with analog electronics and Oliver Gerberding and Katharina-Sophie Isleif for their continued cooperation in the project. M.D.A. would like to thank Olaf Hartwig for fruitful discussions on time-domain stability analysis. This work was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) Project-ID 434617780-SFB 1464. We acknowledge support from the DFG Sonderforschungsbereich 1128 Relativistic Geodesy and Cluster of Excellence “QuantumFrontiers: Light and Matter at the Quantum Frontier: Foundations and Applications in Metrology” (EXC-2123, Project No. 390837967) and the Max Planck Society (MPS) through the LEGACY cooperation on low-frequency gravitational-wave astronomy (M.IF.A.QOP18098). We also acknowledge support by the German Aerospace Center (DLR) with funds from the Federal Ministry of Economics and Technology (BMWi), according to a decision of the German Federal Parliament (Grant No. 50OQ2301, based on Grants No. 50OQ0601, No. 50OQ1301, and No. 50OQ1801).",
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T1 - 2×10-13 Fractional Laser-Frequency Stability with a 7-cm Unequal-Arm Mach-Zehnder Interferometer

AU - Huarcaya, Victor

AU - Álvarez, Miguel Dovale

AU - Penkert, Daniel

AU - Gozzo, Stefano

AU - Cano, Pablo Martínez

AU - Yamamoto, Kohei

AU - Delgado, Juan José Esteban

AU - Mehmet, Moritz

AU - Danzmann, Karsten

AU - Heinzel, Gerhard

N1 - Funding Information: We would like to thank Germán Fernández Barranco for his help with analog electronics and Oliver Gerberding and Katharina-Sophie Isleif for their continued cooperation in the project. M.D.A. would like to thank Olaf Hartwig for fruitful discussions on time-domain stability analysis. This work was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) Project-ID 434617780-SFB 1464. We acknowledge support from the DFG Sonderforschungsbereich 1128 Relativistic Geodesy and Cluster of Excellence “QuantumFrontiers: Light and Matter at the Quantum Frontier: Foundations and Applications in Metrology” (EXC-2123, Project No. 390837967) and the Max Planck Society (MPS) through the LEGACY cooperation on low-frequency gravitational-wave astronomy (M.IF.A.QOP18098). We also acknowledge support by the German Aerospace Center (DLR) with funds from the Federal Ministry of Economics and Technology (BMWi), according to a decision of the German Federal Parliament (Grant No. 50OQ2301, based on Grants No. 50OQ0601, No. 50OQ1301, and No. 50OQ1801).

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N2 - To achieve subpicometer sensitivities in the millihertz band, laser interferometric inertial sensors rely on some form of reduction of the laser-frequency noise, typically by locking the laser to a stable frequency reference, such as the narrow-line-width resonance of an ultrastable optical cavity or an atomic or molecular transition. In this paper, we report on a compact laser-frequency stabilization technique based on an unequal-arm Mach-Zehnder interferometer that is subnanometer stable at 10μHz, subpicometer at 0.5 mHz, and reaches a noise floor of 7fm/Hz at 1 Hz. The interferometer is used in conjunction with a dc servo to stabilize the frequency of a laser down to a fractional instability below 4×10-13 at averaging times from 0.1 to 100 s. The technique offers a wide operating range, does not rely on complex lock-acquisition procedures, and can be readily integrated as part of the optical bench in future gravity missions.

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