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Quantum Enhanced Balanced Heterodyne Readout for Differential Interferometry
Australian Natl Univ, Ctr Gravitat Astrophys, Res Sch Phys, OzGrav, Canberra, ACT, Australia.;Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT, Australia..
KTH, School of Engineering Sciences (SCI), Applied Physics.ORCID iD: 0000-0003-4955-6280
Australian Natl Univ, Ctr Gravitat Astrophys, Res Sch Phys, OzGrav, Canberra, ACT, Australia.;Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT, Australia..
Australian Natl Univ, Ctr Gravitat Astrophys, Res Sch Phys, OzGrav, Canberra, ACT, Australia.;Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT, Australia.;Leibniz Univ Hannover, Inst Gravitat Phys, Hannover, Germany.;Max Planck Inst Grav Phys, Albert Einstein Inst, Hannover, Germany..
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2024 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 133, no 6, article id 063602Article in journal (Refereed) Published
Abstract [en]

Conventional heterodyne readout schemes are now under reconsideration due to the realization of techniques to evade its inherent 3 dB signal-to-noise penalty. The application of high-frequency, quadratureentangled, two-mode squeezed states can further improve the readout sensitivity of audio-band signals. In this Letter, we experimentally demonstrate quantum-enhanced heterodyne readout of two spatially distinct interferometers with direct optical signal combination, circumventing the 3 dB heterodyne signal-to-noise penalty. Applying a high-frequency, quadrature-entangled, two-mode squeezed state, we show further signalto-noise improvement of an injected audio band signal of 3.5 dB. This technique is applicable for quantumlimited high-precision experiments, with application to searches for quantum gravity, searches for dark matter, gravitational wave detection, and wavelength-multiplexed quantum communication.

Place, publisher, year, edition, pages
American Physical Society (APS) , 2024. Vol. 133, no 6, article id 063602
National Category
Atom and Molecular Physics and Optics
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URN: urn:nbn:se:kth:diva-353185DOI: 10.1103/PhysRevLett.133.063602ISI: 001301322400006PubMedID: 39178444Scopus ID: 2-s2.0-85200914768OAI: oai:DiVA.org:kth-353185DiVA, id: diva2:1898493
Note

QC 20240917

Available from: 2024-09-17 Created: 2024-09-17 Last updated: 2024-09-17Bibliographically approved

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Adya, Vaishali

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