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Scalable, symmetric atom interferometer for infrasound gravitational wave detection

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arxiv 1909.01951 v1 pith:P7KMOEHE submitted 2019-09-04 quant-ph

C. Schubert , D. Schlippert , S. Abend , E. Giese , A. Roura , W. P. Schleich , W. Ertmer , E. M. Rasel This is my paper · ORCID
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keywords atomgravitationalinterferometersymmetricwaveachieveadvantagesantennas
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abstract

We propose a terrestrial detector for gravitational waves with frequencies between 0.3 Hz and 5 Hz. Therefore, we discuss a symmetric matter-wave interferometer with a single loop and a folded triple-loop geometry. The latter eliminates the need for atomic ensembles at femtokelvin energies imposed by the Sagnac effect in other atom interferometric detectors. It also combines several advantages of current vertical and horizontal matter wave antennas and enhances the scalability in order to achieve a peak strain sensitivity of $2\cdot10^{-21}\,/\sqrt{\mathrm{Hz}}$.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Massive graviton dark matter searches with long-baseline atom interferometers

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Long-baseline atom interferometers could detect ultra-light spin-2 dark matter through three coupling channels, reaching mass and coupling ranges that LIGO and LISA cannot cover.

  2. Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop

    hep-ex 2024-12 unverdicted novelty 3.0 of 10

    A workshop summary that compiles physics targets, technology advances, and a proto-collaboration roadmap for kilometer-scale atom interferometers aimed at dark matter and gravitational wave detection.

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