Karl Toland, Graeme A R Eddolls, Imogen A Birney, Alan V Cumming, Chalisa Gier, Giles D Hammond, Karen Haughian, James Hough, Russell Jones, Gregoire Lacaille, Iain W Martin, Mariela Masso Reid, Stuart Reid, Sheila Rowan and Gavin Wallace
{"title":"Design and development of a prototype single crystalline silicon cryogenic suspension for 3rd generation gravitational wave detectors","authors":"Karl Toland, Graeme A R Eddolls, Imogen A Birney, Alan V Cumming, Chalisa Gier, Giles D Hammond, Karen Haughian, James Hough, Russell Jones, Gregoire Lacaille, Iain W Martin, Mariela Masso Reid, Stuart Reid, Sheila Rowan and Gavin Wallace","doi":"10.1088/1361-6382/adf8a9","DOIUrl":null,"url":null,"abstract":"Current generation gravitational wave detectors rely on ultra-high purity fused silica in the final monolithic stage of the mirror suspension systems for their excellent thermal noise performance. There is however a push to develop cryogenic suspension systems for the next generation detectors, where fused silica loses its superior thermal noise properties. Silicon is an attractive candidate material, and is the baseline design selected for use in the cryogenic Einstein Telescope and brings with it a new set of challenges. This paper outlines what the authors believe to be the world’s first demonstration of a single ribbon hydroxy-catalysis bonded silicon suspension that has cycled between room temperature and a 4 K environment. Also discussed is the characterisation of similar silicon ribbon, detailing work on surface treatments used to improve the ultimate tensile strength alongside the thermal conductivity of the silicon suspension.","PeriodicalId":10282,"journal":{"name":"Classical and Quantum Gravity","volume":"11 1","pages":""},"PeriodicalIF":3.7000,"publicationDate":"2025-08-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Classical and Quantum Gravity","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1088/1361-6382/adf8a9","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Current generation gravitational wave detectors rely on ultra-high purity fused silica in the final monolithic stage of the mirror suspension systems for their excellent thermal noise performance. There is however a push to develop cryogenic suspension systems for the next generation detectors, where fused silica loses its superior thermal noise properties. Silicon is an attractive candidate material, and is the baseline design selected for use in the cryogenic Einstein Telescope and brings with it a new set of challenges. This paper outlines what the authors believe to be the world’s first demonstration of a single ribbon hydroxy-catalysis bonded silicon suspension that has cycled between room temperature and a 4 K environment. Also discussed is the characterisation of similar silicon ribbon, detailing work on surface treatments used to improve the ultimate tensile strength alongside the thermal conductivity of the silicon suspension.
期刊介绍:
Classical and Quantum Gravity is an established journal for physicists, mathematicians and cosmologists in the fields of gravitation and the theory of spacetime. The journal is now the acknowledged world leader in classical relativity and all areas of quantum gravity.