Rev Sci Instrum
December 2024
High purity silicon is considered as the test mass material for future cryogenic gravitational-wave detectors, in particular Einstein Telescope-low frequency and LIGO Voyager [(LIGO) Laser Interferometer Gravitational-Wave Observatory]. To reduce the thermal noise of the test masses, it is necessary to study the sources of corresponding losses. Mechanical resonators with frequencies 300 Hz-6 kHz are successfully used for studying, for example, losses in optical coatings of the test mass.
View Article and Find Full Text PDFObjective: The aim of this non-inferiority randomised trial was to compare the short and midterm safety and efficacy of hybrid repair (HR) and open reconstruction (OR) for patients with co-existing iliac and common femoral artery (CFA) occlusive disease.
Methods: The study was registered on the ClinicalTrials.gov register (identifier: NCT02580084).
Several projects of the next generation gravitational-wave detectors use the high purity monocrystalline silicon test masses. The electric field of the actuator that is applied to correct the position of the silicon test mass causes additional mechanical losses and associated noise. Disk mechanical resonators are widely used to study mechanical losses in multilayer optical coatings that are deposited on the test masses of gravitational-wave detectors.
View Article and Find Full Text PDFUnlabelled: was to develop a technology for repairing an osteomyelitic bone defect using autologous adipose tissue mesenchymal stromal cells (MSCs) bound to a collagen matrix and to test the efficacy of this technique.
Materials And Methods: The study was carried out with 17 rabbits. A bone defect was created using a milling cutter applied to the proximal third of the leg.