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Photo-oscillations in MgZnO/ZnO heterostructures

We theoretically examine the characteristics of microwave-induced magnetoresistance (MIRO) and photovoltage oscillations in MgZno/ZnO heterostructures. We demonstrate that both kind of oscillations, although described with different physical properties, are intimately related sharing the same physic...

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Autor principal: Iñarrea, Jesús
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9797542/
https://www.ncbi.nlm.nih.gov/pubmed/36577777
http://dx.doi.org/10.1038/s41598-022-27091-0
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author Iñarrea, Jesús
author_facet Iñarrea, Jesús
author_sort Iñarrea, Jesús
collection PubMed
description We theoretically examine the characteristics of microwave-induced magnetoresistance (MIRO) and photovoltage oscillations in MgZno/ZnO heterostructures. We demonstrate that both kind of oscillations, although described with different physical properties, are intimately related sharing the same physical origin. We use the radiation driven electron orbit model showing that the interplay of radiation driven swinging Landau orbits and the scattering processes are at the heart of the oscillations in both scenarios. Thus, our simulations show that all photo-oscillations present the main features of MIRO: they are periodic with the inverse of the magnetic field and the oscillations minima are 1/4 cycle shifted.
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spelling pubmed-97975422022-12-30 Photo-oscillations in MgZnO/ZnO heterostructures Iñarrea, Jesús Sci Rep Article We theoretically examine the characteristics of microwave-induced magnetoresistance (MIRO) and photovoltage oscillations in MgZno/ZnO heterostructures. We demonstrate that both kind of oscillations, although described with different physical properties, are intimately related sharing the same physical origin. We use the radiation driven electron orbit model showing that the interplay of radiation driven swinging Landau orbits and the scattering processes are at the heart of the oscillations in both scenarios. Thus, our simulations show that all photo-oscillations present the main features of MIRO: they are periodic with the inverse of the magnetic field and the oscillations minima are 1/4 cycle shifted. Nature Publishing Group UK 2022-12-28 /pmc/articles/PMC9797542/ /pubmed/36577777 http://dx.doi.org/10.1038/s41598-022-27091-0 Text en © The Author(s) 2022 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Article
Iñarrea, Jesús
Photo-oscillations in MgZnO/ZnO heterostructures
title Photo-oscillations in MgZnO/ZnO heterostructures
title_full Photo-oscillations in MgZnO/ZnO heterostructures
title_fullStr Photo-oscillations in MgZnO/ZnO heterostructures
title_full_unstemmed Photo-oscillations in MgZnO/ZnO heterostructures
title_short Photo-oscillations in MgZnO/ZnO heterostructures
title_sort photo-oscillations in mgzno/zno heterostructures
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9797542/
https://www.ncbi.nlm.nih.gov/pubmed/36577777
http://dx.doi.org/10.1038/s41598-022-27091-0
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