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Negative radiation pressure scheme for simultaneous suppression of arduous back-action evasion and shot noise in gravitational wave detectors

 
cris.virtual.department#PLACEHOLDER_PARENT_METADATA_VALUE#
cris.virtual.department#PLACEHOLDER_PARENT_METADATA_VALUE#
cris.virtual.department#PLACEHOLDER_PARENT_METADATA_VALUE#
cris.virtual.orcid0000-0003-0215-5033
cris.virtual.orcid#PLACEHOLDER_PARENT_METADATA_VALUE#
cris.virtual.orcid0000-0002-9863-2203
cris.virtualsource.departmente7cacdac-f010-492e-846d-bce6f98e4f41
cris.virtualsource.department200d17ab-e3a3-4c08-a7d9-3a32c8397539
cris.virtualsource.department42371cc6-a25b-4311-9c76-8391f7d8ed97
cris.virtualsource.orcide7cacdac-f010-492e-846d-bce6f98e4f41
cris.virtualsource.orcid200d17ab-e3a3-4c08-a7d9-3a32c8397539
cris.virtualsource.orcid42371cc6-a25b-4311-9c76-8391f7d8ed97
dc.contributor.authorAgasti, Souvik
dc.contributor.authorShukla, Abhishek
dc.contributor.authorNesladek, Milos
dc.contributor.imecauthorAgasti, Souvik
dc.contributor.imecauthorShukla, Abhishek
dc.contributor.imecauthorNesladek, Milos
dc.contributor.orcidimecAgasti, Souvik::0000-0002-9863-2203
dc.contributor.orcidimecNesladek, Milos::0000-0003-0215-5033
dc.date.accessioned2025-03-14T18:11:33Z
dc.date.available2025-03-14T18:11:33Z
dc.date.issued2025
dc.description.abstractAiming at applications for gravitational wave (GW) detection, in particular at the reduction of quantum back action noise, we propose a novel scheme how to obtain back action evading measurements performed on an opto-mechanical cavity, by introducing a negative radiation pressure coupling between the cavity field and the end mirror. The scheme consists of introducing a double cavity with end mirrors interlocked by a pivot and moving in opposite directions. The measurement is performed by sending a two-mode squeezed vacuum to both cavities and detecting the output through the heterodyne detection. Compared to the previously proposed hybrid negative mass spin-optomechanical system in Khalili and Polzik (2018 Phys. Rev. Lett. 121 031101), we see that our scheme is capable to suppress back action noise by nearly two orders of magnitude more in the lower frequency region. Overall, the setup has been able to squeeze the output noise below the standard quantum limit, with more efficiency. The scheme has also proven to be beneficial for reducing thermal noise by a significant amount. We confirm our result by a numerical analysis and compared it with the previous proposals (Khalili and Polzik 2018 Phys. Rev. Lett. 121 031101).
dc.description.wosFundingTextS A would like to thank Stefan Danilishin for his fruitful suggestions. The work has been supported by the E-Test (EMR) project, and Horizon Europe Framework Programme (HORIZON-MSCA-2021) Marie Sklodowska-Curie Actions (101065991, SingletSQL).
dc.identifier.doi10.1088/1361-6382/adba37
dc.identifier.issn0264-9381
dc.identifier.urihttps://imec-publications.be/handle/20.500.12860/45397
dc.publisherIOP Publishing Ltd
dc.source.beginpage065021
dc.source.issue6
dc.source.journalCLASSICAL AND QUANTUM GRAVITY
dc.source.numberofpages14
dc.source.volume42
dc.title

Negative radiation pressure scheme for simultaneous suppression of arduous back-action evasion and shot noise in gravitational wave detectors

dc.typeJournal article
dspace.entity.typePublication
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