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20162025
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 1.2k across the 37 of their papers we have counts for

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Showing 2020Show all

9 papers · 1 filter

gr-qc2020★ 10 cited

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-qc2020★ 2 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-qc2020★ 23 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…

astro-ph.IM2020★ 5 cited

Demonstration of a dual-pass differential Fabry-Perot interferometer for future interferometric space gravitational wave antennas

Koji Nagano, Hiroki Takeda, Yuta Michimura +2

A dual-pass differential Fabry-Perot interferometer (DPDFPI) is one candidate of the interferometer configurations utilized in future Fabry-Perot type space gravitational wave ante…

gr-qc2020★ 9 cited

Overview of KAGRA : KAGRA science

KAGRA Collaboration, T. Akutsu, M. Ando +240

KAGRA is a newly build gravitational-wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper in the series of KAGRA-featured a…

gr-qc2020★ 23 cited

Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA

Yuta Michimura, Kentaro Komori, Yutaro Enomoto +18

Upgrades to improve the sensitivity of gravitational wave detectors enable more frequent detections and more precise source parameter estimation. Unlike other advanced interferomet…

quant-ph2020★ 5 cited

Optical trapping of the transversal motion for an optically levitated mirror

Takuya Kawasaki, Naoki Kita, Koji Nagano +4

Optomechanical systems are suitable for elucidating quantum phenomena at the macroscopic scale in the sense of the mass scale. The systems should be well-isolated from the environm…

gr-qc2020

Current status of space gravitational wave antenna DECIGO and B-DECIGO

Seiji Kawamura, Masaki Ando, Naoki Seto +84

Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO) is the future Japanese space mission with a frequency band of 0.1 Hz to 10 Hz. DECIGO aims at the detection of pri…

gr-qc2020★ 16 cited

Optimization of quantum noise by completing the square of multiple interferometer outputs in quantum locking for gravitational wave detectors

Rika Yamada, Yutaro Enomoto, Atsushi Nishizawa +11

The quantum locking technique, which uses additional short low-loss sub-cavities, is effective in reducing quantum noise in space gravitational wave antenna DECIGO. However, the qu…