Proof-of-principle experiment on a displacement-noise-free neutron interferometer for gravitational wave detection

The displacement-noise-free interferometer (DFI) is designed to eliminate all displacement-induced noise while retaining sensitivity to gravitational wave (GW) signals. Ground-based DFIs suffer from physical arm-length limitations, resulting in poor sensitivity at frequencies below 1 kHz. To address this, previous research introduced a neutron-based DFI, which replaces laser light with neutrons and achieves exceptional sensitivity down to a few hertz. In this study, we conducted a proof-of-principle experiment using a pulsed neutron source at the Japan Proton Accelerator Research Complex. Despite practical constraints that led to deviations from the ideal experimental design, we optimized the setup and developed a novel analysis method that successfully cancels displacement noise while preserving simulated GW signals. This work presents the first successful demonstration of a neutron DFI and a neutron interferometer for GW detection.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-11-06
DOI
https://doi.org/10.1103/yg4l-cj1t
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
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article

Proof-of-principle experiment on a displacement-noise-free neutron interferometer for gravitational wave detection

Seiji Kawamura, Yuta Michimura, K. Mishima, Masaaki Kitaguchi et al.
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
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Proof-of-principle experiment on a displacement-noise-free neutron interferometer for gravitational wave detection

Seiji Kawamura, Yuta Michimura, K. Mishima, Masaaki Kitaguchi, Tomohiro Ishikawa, Takuhiro Fujiie, Takafumi Onishi, K. Kokeyama, T. Nambu, Kazuhiro Kobayashi, Shoki Iwaguchi, A. Nishizawa, Hirohiko M. Shimizu, Kurumi Umemura, Yutaka Yamagata, Kenji Tsuji
article en

Abstract

The displacement-noise-free interferometer (DFI) is designed to eliminate all displacement-induced noise while retaining sensitivity to gravitational wave (GW) signals. Ground-based DFIs suffer from physical arm-length limitations, resulting in poor sensitivity at frequencies below 1 kHz. To address this, previous research introduced a neutron-based DFI, which replaces laser light with neutrons and achieves exceptional sensitivity down to a few hertz. In this study, we conducted a proof-of-principle experiment using a pulsed neutron source at the Japan Proton Accelerator Research Complex. Despite practical constraints that led to deviations from the ideal experimental design, we optimized the setup and developed a novel analysis method that successfully cancels displacement noise while preserving simulated GW signals. This work presents the first successful demonstration of a neutron DFI and a neutron interferometer for GW detection.

Physical review. D/Physical review. D.Vol. 112(10)
Hiroshima University (JP), Obayashi (Japan) (JP), Rikkyo University (JP), High Energy Accelerator Research Organization (JP), Kavli Institute for the Physics and Mathematics of the Universe (JP), RIKEN Center for Advanced Photonics (JP), Nagoya University (JP), The University of Tokyo (JP), Cardiff University (GB)
Openalex Percentile: Top 77%
Pulsars and Gravitational Waves Research
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