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- W3204810846 abstract "Gravitational waves are most simply thought of as ripples in the curvature of space-time, their effect being to change the separation of adjacent masses on earth or in space; this tidal effect is the basis of all present detectors. The necessity of being able to detect such small signal levels means that noise, resulting from a variety of sources, such as the thermal motion of molecules in the detector, from seismic or other mechanical disturbances, and from noise associated with the detector readout, whether electronic or optical, must be reduced to a very low level. An alternative design of gravitational wave detector offers the possibility of very high sensitivities over a wide range of frequency. Fundamentally it should be possible to build systems using laser interferometry to monitor strains in space which are limited only by the Heisenberg Uncertainty Principle; however there are other practical issues which must be taken into account." @default.
- W3204810846 created "2021-10-11" @default.
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- W3204810846 date "2021-09-23" @default.
- W3204810846 modified "2023-09-24" @default.
- W3204810846 title "Lasers for interferometric gravitational wave detectors" @default.
- W3204810846 doi "https://doi.org/10.1201/9781003209652-11" @default.
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