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dc.contributor.authorPaniagua-Diaz, AM
dc.contributor.authorBarnes, WL
dc.contributor.authorBertolotti, J
dc.date.accessioned2023-04-24T12:58:25Z
dc.date.issued2023-02-22
dc.date.updated2023-04-24T10:52:46Z
dc.description.abstractA perfectly collimated beam can be spread out by multiple scattering, creating a speckle pattern and increasing the étendue of the system. Standard optical systems conserve étendue, and thus are unable to reverse the process by transforming a speckle pattern into a collimated beam or, equivalently, into a sharp focus. Wavefront shaping is a technique that is able to manipulate the amplitude and/or phase of a light beam, thus controlling its propagation through such media. Wavefront shaping can thus break the conservation of étendue and, in principle, reduce it. In this work we study how much of the energy contained in a fully developed speckle pattern can be converted into a high quality (low M 2) beam, we support it with a theoretical framework and discuss the advantages and limitations of this approach.en_GB
dc.format.extent035516-
dc.identifier.citationVol. 98(3), article 035516en_GB
dc.identifier.doihttps://doi.org/10.1088/1402-4896/acbbab
dc.identifier.urihttp://hdl.handle.net/10871/132998
dc.identifierORCID: 0000-0002-9474-5534 (Barnes, WL)
dc.identifierORCID: 0000-0002-7163-6343 (Bertolotti, J)
dc.language.isoenen_GB
dc.publisherIOP Publishing / Royal Swedish Academy of Sciencesen_GB
dc.relation.urlhttps://doi.org/10.5281/zenodo.4964616en_GB
dc.rights.embargoreasonUnder embargo until 22 February 2024 in compliance with publisher policyen_GB
dc.rights© 2023 IOP Publishing Ltd. This version is made available under the CC-BY-NC-ND 4.0 license: https://creativecommons.org/licenses/by-nc-nd/4.0/  en_GB
dc.subjectwavefront shapingen_GB
dc.subjectmultiple scatteringen_GB
dc.subjecthigh power lasersen_GB
dc.titleWavefront shaping to improve beam quality: converting a speckle pattern into a Gaussian spoten_GB
dc.typeArticleen_GB
dc.date.available2023-04-24T12:58:25Z
dc.identifier.issn0031-8949
exeter.article-numberARTN 035516
dc.descriptionThis is the author accepted manuscript. The final version is available from IOP Publishing via the DOI in this recorden_GB
dc.descriptionData availability statement: The data that support the findings of this study are openly available at the following URL/DOI: https://doi.org/10.5281/zenodo.4964616en_GB
dc.identifier.eissn1402-4896
dc.identifier.journalPhysica Scriptaen_GB
dc.relation.ispartofPhysica Scripta, 98(3)
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/  en_GB
dcterms.dateAccepted2023-02-13
rioxxterms.versionAMen_GB
rioxxterms.licenseref.startdate2023-02-22
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2023-04-24T12:55:29Z
refterms.versionFCDAM
refterms.dateFOA2024-02-22T00:00:00Z
refterms.panelBen_GB
refterms.dateFirstOnline2023-02-22


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© 2023 IOP Publishing Ltd. This version is made available under the CC-BY-NC-ND 4.0 license: https://creativecommons.org/licenses/by-nc-nd/4.0/  
Except where otherwise noted, this item's licence is described as © 2023 IOP Publishing Ltd. This version is made available under the CC-BY-NC-ND 4.0 license: https://creativecommons.org/licenses/by-nc-nd/4.0/