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

23 citations · 25 across the 2 of their papers we have counts for

collaborators

5 papers

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…

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

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…