Abstract

Low-losses and directionality effects exhibited by High Refractive Index Dielectric particles make them attractive for applications where radiation direction control is relevant. For instance, isolated metallo-dielectric core-shell particles or aggregates (dimers) of High Refractive Index Dielectric particles have been proposed for building operational switching devices. Also, the possibility of using isolated High Refractive Index Dielectric particles for optimizing solar cells performance has been explored. Here, we present experimental evidence in the microwave range, that a High Refractive Index Dielectric dimer of spherical particles is more efficient for redirecting the incident radiation in the forward direction than the isolated case. In fact, we report two spectral regions in the dipolar spectral range where the incident intensity is mostly scattered in the forward direction. They correspond to the Zero-Backward condition (also observed for isolated particles) and to a new condition, denoted as “near Zero-Backward” condition, which comes from the interaction effects between the particles. The proposed configuration has implications in solar energy harvesting devices and in radiation guiding.

Details

Title
On the scattering directionality of a dielectric particle dimer of High Refractive Index
Author
Barreda, Ángela I 1 ; Saleh, Hassan 2 ; Litman, Amélie 3 ; González, Francisco 1 ; Jean-Michel Geffrin 3   VIAFID ORCID Logo  ; Moreno, Fernando 1 

 Group of Optics, Department of Applied Physics, University of Cantabria, Cantabria, Spain 
 Aix-Marseille Univ, CNRS, Centrale Marseille, Institut Fresnel, Marseille, France; Centre Commun de Ressources en Microondes CCRM, 5 rue Enrico Fermi, Marseille, France 
 Aix-Marseille Univ, CNRS, Centrale Marseille, Institut Fresnel, Marseille, France 
Pages
1-12
Publication year
2018
Publication date
May 2018
Publisher
Nature Publishing Group
e-ISSN
20452322
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2042728820
Copyright
© 2018. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.