Pramana | |
Physics of interferometric gravitational wave detectors | |
Biplab Bhawal11  | |
[1] LIGO Laboratory, California Institute of Technology, Pasadena, CA 91125, USA$$ | |
关键词: Interferometer; gravitational wave; Laser Interferometer Gravitational-wave Observatory.; | |
DOI : | |
学科分类:物理(综合) | |
来源: Indian Academy of Sciences | |
【 摘 要 】
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and two of 4 km) in order to unambiguously measure the infinitesimal displacements of isolated test masses which convey the signature of gravitational waves from astrophysical sources. An interferometric gravitational wave detector like LIGO is a complex, non-linear, coupled, dynamic system. This article summarizes various interesting design characteristics of these detectors and techniques that were implemented in order to reach and maintain its operating condition. Specifically, the following topics are discussed:length sensing and control,
【 授权许可】
Unknown
【 预 览 】
Files | Size | Format | View |
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RO201912040496708ZK.pdf | 578KB | download |