Observation of strong nonlinear interactions in parametric down-conversion of X-rays into ultraviolet radiation.


Journal

Nature communications
ISSN: 2041-1723
Titre abrégé: Nat Commun
Pays: England
ID NLM: 101528555

Informations de publication

Date de publication:
12 12 2019
Historique:
received: 14 04 2019
accepted: 18 11 2019
entrez: 14 12 2019
pubmed: 14 12 2019
medline: 14 12 2019
Statut: epublish

Résumé

Nonlinear interactions between X-rays and long wavelength radiation can be used as a powerful atomic-scale probe for light-matter interactions and for properties of valence electrons. However, reported X-ray nonlinear effects were small and their observations required tremendous efforts. Here we report the observation of strong nonlinearities in parametric down-conversion (PDC) of X-rays to long wavelength radiation in gallium arsenide and lithium niobate crystals, with efficiencies about 4 orders of magnitude stronger than the efficiencies measured in any material studied before. Furthermore, we show that the efficiency in the ferroelectric phase of strontium barium niobite is two orders of magnitude stronger than in its paraelectric phase. This observation suggests that the lack of inversion symmetry is the origin for the strong observed nonlinearity. Additionally, we demonstrate the ability to use the effect for the investigation of the spectral response of non-centrosymmetric materials at wavelengths ranging from infrared to soft X-rays.

Identifiants

pubmed: 31831734
doi: 10.1038/s41467-019-13629-w
pii: 10.1038/s41467-019-13629-w
pmc: PMC6908627
doi:

Types de publication

Journal Article Research Support, Non-U.S. Gov't

Langues

eng

Sous-ensembles de citation

IM

Pagination

5673

Références

Phys Rev Lett. 2018 Aug 24;121(8):083901
pubmed: 30192600
Proc Natl Acad Sci U S A. 2016 Feb 9;113(6):1492-7
pubmed: 26811449
Phys Rev Lett. 2019 Jan 18;122(2):023902
pubmed: 30720320
Opt Express. 2015 Mar 23;23(6):7471-80
pubmed: 25837087
Nature. 2012 Aug 30;488(7413):603-8
pubmed: 22932384
Phys Rev Lett. 2007 Jun 15;98(24):244801
pubmed: 17677969
Phys Rev Lett. 2007 Oct 19;99(16):163001
pubmed: 17995246
Phys Rev Lett. 2017 Dec 22;119(25):253902
pubmed: 29303339
Phys Rev Lett. 2009 Dec 18;103(25):254801
pubmed: 20366257
Phys Rev Lett. 2018 Jun 15;120(24):243902
pubmed: 29956957

Auteurs

S Sofer (S)

Physics Department and Institute of Nanotechnology, Bar-Ilan University, 52900, Ramat Gan, Israel.

O Sefi (O)

Physics Department and Institute of Nanotechnology, Bar-Ilan University, 52900, Ramat Gan, Israel.

E Strizhevsky (E)

Physics Department and Institute of Nanotechnology, Bar-Ilan University, 52900, Ramat Gan, Israel.

H Aknin (H)

Physics Department and Institute of Nanotechnology, Bar-Ilan University, 52900, Ramat Gan, Israel.

S P Collins (SP)

Diamond Light Source, Harwell Science and Innovation Campus, Didcot, OX11 0DE, UK.

G Nisbet (G)

Diamond Light Source, Harwell Science and Innovation Campus, Didcot, OX11 0DE, UK.

B Detlefs (B)

ESRF-The European Synchrotron, CS 40220, 38043, Grenoble, Cedex 9, France.

Ch J Sahle (CJ)

ESRF-The European Synchrotron, CS 40220, 38043, Grenoble, Cedex 9, France.

S Shwartz (S)

Physics Department and Institute of Nanotechnology, Bar-Ilan University, 52900, Ramat Gan, Israel. sharon.shwartz@biu.ac.il.

Classifications MeSH