{"title":"作为引力波探测器的弹性棒和弹性旋转环","authors":"José Natário, Amol Sasane, Rodrigo Vicente","doi":"arxiv-2407.07547","DOIUrl":null,"url":null,"abstract":"Linearised relativistic elasticity equations of motion are considered for a\nrod and a spinning ring encountering a gravitational wave. In the case of the\nrod, the equations reduce to a wave equation with appropriate boundary\nconditions. Using Fourier transforms, the resonant frequencies are found and an\nexplicit distributional solution is given, both for a plus- and a\ncross-polarised gravitational wave. In the case of the spinning ring, the\nequations are coupled wave equations with periodic boundary conditions. Using a\nFourier series expansion, the system of wave equations is recast as a family of\nordinary differential equations for the Fourier coefficients, which are then\nsolved via Fourier transforms. The resonant frequencies are found, including\nsimple approximate expressions for slowly rotating rings, and an explicit\ndistributional solution is obtained in the case of the non-spinning ring.\nInterestingly, it is possible to tune the resonant frequencies by adjusting the\nangular velocity of the spinning ring.","PeriodicalId":501482,"journal":{"name":"arXiv - PHYS - Classical Physics","volume":"71 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Elastic rods and elastic spinning rings as gravitational wave detectors\",\"authors\":\"José Natário, Amol Sasane, Rodrigo Vicente\",\"doi\":\"arxiv-2407.07547\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Linearised relativistic elasticity equations of motion are considered for a\\nrod and a spinning ring encountering a gravitational wave. In the case of the\\nrod, the equations reduce to a wave equation with appropriate boundary\\nconditions. Using Fourier transforms, the resonant frequencies are found and an\\nexplicit distributional solution is given, both for a plus- and a\\ncross-polarised gravitational wave. In the case of the spinning ring, the\\nequations are coupled wave equations with periodic boundary conditions. Using a\\nFourier series expansion, the system of wave equations is recast as a family of\\nordinary differential equations for the Fourier coefficients, which are then\\nsolved via Fourier transforms. The resonant frequencies are found, including\\nsimple approximate expressions for slowly rotating rings, and an explicit\\ndistributional solution is obtained in the case of the non-spinning ring.\\nInterestingly, it is possible to tune the resonant frequencies by adjusting the\\nangular velocity of the spinning ring.\",\"PeriodicalId\":501482,\"journal\":{\"name\":\"arXiv - PHYS - Classical Physics\",\"volume\":\"71 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-07-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Classical Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2407.07547\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Classical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2407.07547","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Elastic rods and elastic spinning rings as gravitational wave detectors
Linearised relativistic elasticity equations of motion are considered for a
rod and a spinning ring encountering a gravitational wave. In the case of the
rod, the equations reduce to a wave equation with appropriate boundary
conditions. Using Fourier transforms, the resonant frequencies are found and an
explicit distributional solution is given, both for a plus- and a
cross-polarised gravitational wave. In the case of the spinning ring, the
equations are coupled wave equations with periodic boundary conditions. Using a
Fourier series expansion, the system of wave equations is recast as a family of
ordinary differential equations for the Fourier coefficients, which are then
solved via Fourier transforms. The resonant frequencies are found, including
simple approximate expressions for slowly rotating rings, and an explicit
distributional solution is obtained in the case of the non-spinning ring.
Interestingly, it is possible to tune the resonant frequencies by adjusting the
angular velocity of the spinning ring.