Optimisation of table-top 3D interferometers for Observational Quantum Gravity

• DOI: 10.48550/arxiv.2105.09664
• Publication Date: 2021-01-01
• Authors: Griffiths, Willia...; Aiello, Lorenzo; Ejlli, Aldo; James, Alasdair L.; Vermeulen, Sander M.; Dooley, Katherine L.; Grote, Hartmut
• Keywords: 0103 physical sciences; FOS: Physical sciences; General Relativity and Quantum Cosmology (gr-qc); Astrophysics - Instrumentation and Methods for Astrophysics; 01 natural sciences; Instrumentation and Methods for Astrophysics (astro-ph.IM); General Relativity and Quantum Cosmology

With the use of twin, co-located, 3D interferometers, Cardiff University's Gravity Exploration Institute aims to observe quantum fluctuations of space-time as predicted by some theories of quantum gravity. Our design displacement sensitivity exceeds that of previous similar experiments, which have constrained the magnitudes of the fluctuations in the 1-25 MHz band. The increased sensitivity comes in large part from the comparably higher circulating power we aim to achieve, which reduces the overall shot noise. One complication of higher circulating power is an increase in contrast defect light, which includes higher-order modes. We will use the DC-readout scheme, whose dark-fringe offset must sufficiently dominate the contrast defect in order to detect faint signals. However, too much total output power risks saturating the high-bandwidth photodetectors. Suppressing the higher-order mode content of the contrast defect is a key strategy to realising the high circulating power and eliminating non-signal-carrying power that contributes to shot noise. For this, the inclusion of an output mode cleaner, whose design is described, is required.<br/>6 pages, 3 figures, 1 table, Contribution to the 2021 Gravitation session of the 55th Rencontres de Moriond<br/>