期刊
CLASSICAL AND QUANTUM GRAVITY
卷 26, 期 8, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/26/8/085012
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- STFC [PP/F001118/1, PP/E001203/1] Funding Source: UKRI
- Science and Technology Facilities Council [PP/E001203/1, PP/F001118/1] Funding Source: researchfish
The upcoming European design study 'Einstein gravitational-wave Telescope' represents the first step towards a substantial, international effort for the design of a third-generation interferometric gravitational wave detector. It is generally believed that third-generation instruments might not be installed into existing infrastructures but will provoke a new search for optimal detector sites. Consequently, the detector design could be subject to fewer constraints than the on-going design of the second-generation instruments. In particular, it will be prudent to investigate alternatives to the traditional L-shaped Michelson interferometer. In this paper, we review an old proposal to use three Michelson interferometers in a triangular configuration. We use this example of a triple Michelson interferometer to clarify the terminology and will put this idea into the context of more recent research on interferometer technologies. Furthermore, the benefits of a triangular detector will be used to motivate this design as a good starting point for a more detailed research effort towards a third-generation gravitational-wave detector.
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