activity
20182022
most citedImproved sensitivity of interferometric gravitational wave detectors to ultralight vector dark matter from the finite light-traveling time

42 citations · 195 across the 17 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

quant-ph20223 cited

Photothermal effect in macroscopic optomechanical systems with an intracavity nonlinear optical crystal

Sotatsu Otabe, Kentaro Komori, Ken-ichi Harada +3

Intracavity squeezing is a promising technique that may improve the sensitivity of gravitational wave detectors and cool optomechanical oscillators to the ground state. However, th…

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…

astro-ph.CO2022

Stochastic effects on observation of ultralight bosonic dark matter

Hiromasa Nakatsuka, Soichiro Morisaki, Tomohiro Fujita +4

Ultralight bosonic particles are fascinating candidates of dark matter (DM). It behaves as classical waves in our Galaxy due to its large number density. There have been various me…

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…