Dispersion balanced figure-eight laser

Theimer, James P.; Haus, Jörg

doi:10.1016/s0030-4018(96)00511-1

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Some Experimental Proposals For Its Observation1

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Cited by 3 publications

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“…The use of two masses enables a range of experimental conditions to be considered. Anandan and Chaio already favoured a figure-8 ring for a gravitational wave antenna [11], a configuration also considered by others [58,64]. In the equatorial plane we obtain a Lense-Thirring rotation:…”

Section: Some Experimental Proposals For Its Observationsupporting

confidence: 52%

On the detectability of the Lense–Thirring field from rotating laboratory masses using ring laser gyroscope interferometers

Stedman

Schreiber

Bilger

2003

Class. Quantum Grav.

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The possibility of detecting the Lense–Thirring field generated by the rotating earth (also rotating laboratory masses) is reassessed in view of recent dramatic advances in the technology of ring laser gyroscopes. This possibility is very much less remote than it was a decade ago. The effect may contribute significantly to the Sagnac frequency of planned instruments. Its discrimination and detection will require an improved metrology, linking the ring to the celestial reference frame, and a fuller study of dispersion- and backscatter-induced frequency pulling. Both these requirements have been the subject of recent major progress, and our goal looks feasible.

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Section: Some Experimental Proposals For Its Observationsupporting

confidence: 52%