I. Zawischa, S. Knoke, H. Zellmer, A. Tunnermann, H. Welling, O. S. Brozek, K. Danzmann, I. Freitag
{"title":"1064nm高功率低强度噪声单频光源","authors":"I. Zawischa, S. Knoke, H. Zellmer, A. Tunnermann, H. Welling, O. S. Brozek, K. Danzmann, I. Freitag","doi":"10.1109/CLEOE.1998.719166","DOIUrl":null,"url":null,"abstract":"High power low noise lasers are needed in high precision interferometric gravitational wave detection In the GEO-600 gravitational wave detector a relative intensity noise of less than 10-8/√Hz and a frequency stability better than 10-3/√Hz will be required.\n On power levels up to 2 W diode pumped non-planar monolithic Nd: YAG ring lasers (NPRO) are well known for their superior noise properties and their high potential for active stabilisation and intensity noise reduction [1].","PeriodicalId":404067,"journal":{"name":"CLEO/Europe Conference on Lasers and Electro-Optics","volume":"96 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1998-09-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"High Power Low Intensity Noise Single Frequency Light Sources at 1064 nm\",\"authors\":\"I. Zawischa, S. Knoke, H. Zellmer, A. Tunnermann, H. Welling, O. S. Brozek, K. Danzmann, I. Freitag\",\"doi\":\"10.1109/CLEOE.1998.719166\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"High power low noise lasers are needed in high precision interferometric gravitational wave detection In the GEO-600 gravitational wave detector a relative intensity noise of less than 10-8/√Hz and a frequency stability better than 10-3/√Hz will be required.\\n On power levels up to 2 W diode pumped non-planar monolithic Nd: YAG ring lasers (NPRO) are well known for their superior noise properties and their high potential for active stabilisation and intensity noise reduction [1].\",\"PeriodicalId\":404067,\"journal\":{\"name\":\"CLEO/Europe Conference on Lasers and Electro-Optics\",\"volume\":\"96 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1998-09-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"CLEO/Europe Conference on Lasers and Electro-Optics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/CLEOE.1998.719166\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"CLEO/Europe Conference on Lasers and Electro-Optics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/CLEOE.1998.719166","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
High Power Low Intensity Noise Single Frequency Light Sources at 1064 nm
High power low noise lasers are needed in high precision interferometric gravitational wave detection In the GEO-600 gravitational wave detector a relative intensity noise of less than 10-8/√Hz and a frequency stability better than 10-3/√Hz will be required.
On power levels up to 2 W diode pumped non-planar monolithic Nd: YAG ring lasers (NPRO) are well known for their superior noise properties and their high potential for active stabilisation and intensity noise reduction [1].
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