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20182025
most citedImproved sensitivity of interferometric gravitational wave detectors to ultralight vector dark matter from the finite light-traveling time

42 citations · 195 across the 18 of their papers we have counts for

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Showing gr-qcShow all

15 papers · 1 filter

gr-qc2022

Input optics systems of the KAGRA detector during O3GK

T. Akutsu, M. Ando, K. Arai +246

KAGRA, the underground and cryogenic gravitational-wave detector, was operated for its solo observation from February 25th to March 10th, 2020, and its first joint observation with…

gr-qc20221 cited

Can the phase of radiation pressure fluctuations be flipped in a single path for laser interferometric gravitational wave detectors?

Tomohiro Ishikawa, Shoki Iwaguchi, Bin Wu +7

Radiation pressure (RP) noise, one component of quantum noise, can limit the sensitivity of laser interferometric gravitational wave (GW) detectors at lower frequencies. We conceiv…

gr-qc20226 cited

Displacement-noise-free neutron interferometer for gravitational wave detection using a single Mach-Zehnder configuration

Shoki Iwaguchi, Atsushi Nishizawa, Yanbei Chen +10

The improvement of sensitivity to gravitational waves (GWs) at lower frequencies is still challenging on account of displacement noise. One of the solutions is the neutron displace…

gr-qc2020

Reduction of quantum noise using the quantum locking with an optical spring for gravitational wave detectors

Rika Yamada, Yutaro Enomoto, Izumi Watanabe +11

In our previous research, simulation showed that a quantum locking scheme with homodyne detection in sub-cavities is effective in surpassing the quantum noise limit for Deci-hertz…

gr-qc20202 cited

Quantum noise in a Fabry-Perot interferometer including the influence of diffraction loss of light

Shoki. Iwaguchi, Tomohiro. Ishikawa, Masaki. Ando +10

The DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is designed to detect gravitational waves at frequencies between 0.1 and 10 Hz. In this frequency band, one of…

gr-qc202023 cited

Improvement of the target sensitivity in DECIGO by optimizing its parameters for quantum noise including the effect of diffraction loss

Tomohiro Ishikawa, Shoki Iwaguchi, Yuta Michimura +10

DECIGO is the future Japanese gravitational wave detector in outer space. We previously set the default design parameters to provide a good target sensitivity to detect the primord…