activity
20032026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 47.8k across the 251 of their papers we have counts for

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12 papers · 1 filter

physics.ins-det2026

Cryogenic Mechanical Loss of GaAs/AlGaAs Crystalline Coatings

Nicholas A. Didio, Steven D. Penn, Satoshi Tanioka +3

Optical coatings with minimal thermal noise are essential for high-precision, laser-based metrology experiments. Substrate-transferred crystalline GaAs/AlGaAs coa…

physics.ins-det2025

Birefringence of AlGaAs/GaAs Coatings under Above-Band-Gap Illumination, GR Noise and Photo-Optic Transfer Function

Bin Wu, Shreyan Goswami, Satoshi Tanioka +1

AlGaAs/GaAs coatings are being considered as coating candidates for gravitational-wave detectors. In this paper we investigate the birefringence properties of this crystalline semi…

physics.ins-det2024★ 1 cited

Criteria for identifying and evaluating locations that could potentially host the Cosmic Explorer observatories

Kathryne J. Daniel, Joshua R. Smith, Stefan Ballmer +19

Cosmic Explorer (CE) is a next-generation ground-based gravitational-wave observatory that is being designed in the 2020s and is envisioned to begin operations in the 2030s togethe…

physics.ins-det2022★ 7 cited

Study on electro-optic noise in crystalline coatings toward future gravitational wave detectors

Satoshi Tanioka, Daniel Vander-Hyde, Garrett D. Cole +2

Thermal noise in high-reflectivity mirror coatings is a limiting factor in ground-based gravitational wave detectors. Reducing this coating thermal noise improves the sensitivity o…

physics.ins-det2021★ 6 cited

Point Absorber Limits to Future Gravitational-Wave Detectors

W. Jia, H. Yamamoto, K. Kuns +198

High-quality optical resonant cavities require low optical loss, typically on the scale of parts per million. However, unintended micron-scale contaminants on the resonator mirrors…

physics.ins-det2021★ 53 cited

LIGOs Quantum Response to Squeezed States

L. McCuller, S. E. Dwyer, A. C. Green +194

Gravitational Wave interferometers achieve their profound sensitivity by combining a Michelson interferometer with optical cavities, suspended masses, and now, squeezed quantum sta…