Adaptive optical imaging with entangled photons.


Journal

Science (New York, N.Y.)
ISSN: 1095-9203
Titre abrégé: Science
Pays: United States
ID NLM: 0404511

Informations de publication

Date de publication:
08 Mar 2024
Historique:
medline: 7 3 2024
pubmed: 7 3 2024
entrez: 7 3 2024
Statut: ppublish

Résumé

Adaptive optics (AO) has revolutionized imaging in fields from astronomy to microscopy by correcting optical aberrations. In label-free microscopes, however, conventional AO faces limitations because of the absence of a guide star and the need to select an optimization metric specific to the sample and imaging process. Here, we propose an AO approach leveraging correlations between entangled photons to directly correct the point spread function. This guide star-free method is independent of the specimen and imaging modality. We demonstrate the imaging of biological samples in the presence of aberrations using a bright-field imaging setup operating with a source of spatially entangled photon pairs. Our approach performs better than conventional AO in correcting specific aberrations, particularly those involving substantial defocus. Our work improves AO for label-free microscopy and could play a major role in the development of quantum microscopes.

Identifiants

pubmed: 38452085
doi: 10.1126/science.adk7825
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

1142-1148

Auteurs

Patrick Cameron (P)

School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK.

Baptiste Courme (B)

Sorbonne Université, CNRS, Institut des NanoSciences de Paris, INSP, F-75005 Paris, France.
Laboratoire Kastler Brossel, ENS-Universite PSL, CNRS, Sorbonne Universite, College de France, 75005 Paris, France.

Chloé Vernière (C)

Sorbonne Université, CNRS, Institut des NanoSciences de Paris, INSP, F-75005 Paris, France.

Raj Pandya (R)

Sorbonne Université, CNRS, Institut des NanoSciences de Paris, INSP, F-75005 Paris, France.
Laboratoire Kastler Brossel, ENS-Universite PSL, CNRS, Sorbonne Universite, College de France, 75005 Paris, France.
Cavendish Laboratory, University of Cambridge, Cambridge CB3 0HE, UK.

Daniele Faccio (D)

School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK.

Hugo Defienne (H)

School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK.
Sorbonne Université, CNRS, Institut des NanoSciences de Paris, INSP, F-75005 Paris, France.

Classifications MeSH