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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

collaborators
Showing 2020Show all

13 papers · 1 filter

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…

hep-ph202042 cited

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

Soichiro Morisaki, Tomohiro Fujita, Yuta Michimura +2

Recently several studies have pointed out that gravitational-wave detectors are sensitive to ultralight vector dark matter and can improve the current best constraints given by the…

physics.ins-det2020

Cryogenic suspension design for a kilometer-scale gravitational-wave detector

Takafumi Ushiba, Tomotada Akutsu, Yoichi Aso +43

We report the mirror suspension design for Large-scale Cryogenic Gravitational wave Telescope, KAGRA, during bKAGRA Phase 1. Mirror thermal noise is one of the fundamental noises f…

gr-qc20209 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…