Fenollosa Esteve, R.; Ramiro-Manzano, F.; Garín Escrivá, M.; Alcubilla, R. (2019). Thermal Emission of Silicon at Near-Infrared Frequencies Mediated by Mie Resonances. ACS Photonics. 6(12):3174-3179. https://doi.org/10.1021/acsphotonics.9b01513
Por favor, use este identificador para citar o enlazar este ítem: http://hdl.handle.net/10251/150637
Título:
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Thermal Emission of Silicon at Near-Infrared Frequencies Mediated by Mie Resonances
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Autor:
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Fenollosa Esteve, Roberto
Ramiro-Manzano, Fernando
GARÍN ESCRIVÁ, MOISÉS
Alcubilla, R.
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Entidad UPV:
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Universitat Politècnica de València. Centro de Tecnologías Físicas: Acústica, Materiales y Astrofísica - Centre de Tecnologies Físiques: Acústica, Materials i Astrofísica
Universitat Politècnica de València. Instituto Universitario Mixto de Tecnología Química - Institut Universitari Mixt de Tecnologia Química
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Fecha difusión:
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Resumen:
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[EN] Planck's law constitutes one of the cornerstones in physics. It explains the well-known spectrum of an ideal blackbody consisting of a smooth curve, whose peak wavelength and intensity depend on the temperature of the ...[+]
[EN] Planck's law constitutes one of the cornerstones in physics. It explains the well-known spectrum of an ideal blackbody consisting of a smooth curve, whose peak wavelength and intensity depend on the temperature of the body. This scenario changes drastically, however, when the size of the emitting object is comparable to the wavelength of the emitted radiation. Here we show that a silicon microsphere (2-3 mu m in diameter) heated to around 800 degrees C yields a thermal emission spectrum consisting of pronounced peaks that are associated with Mie resonances. We experimentally demonstrate in the near-infrared the existence of modes with an ultrahigh quality factor, Q, of 400, which is substantially higher than values reported so far, and set a new benchmark in the field of thermal emission. Simulations predict that the thermal response of the microspheres is very fast, about 15 mu s. Additionally, the possibility of achieving light emission above the Planck limit at some frequency ranges is envisaged.
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Palabras clave:
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Microsphere
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Silicon
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Nanocavity
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Whispering gallery modes
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Super-Planckian
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Light source
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Derechos de uso:
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Reserva de todos los derechos
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Fuente:
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ACS Photonics. (eissn:
2330-4022
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DOI:
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10.1021/acsphotonics.9b01513
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Editorial:
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American Chemical Society
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Versión del editor:
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https://doi.org/10.1021/acsphotonics.9b01513
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Código del Proyecto:
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info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-099744-B-I00/ES/AMPLIFICACION DE LOS FENOMENOS OPTOELECTRONICOS EN MICROCAVIDADES/
...[+]
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-099744-B-I00/ES/AMPLIFICACION DE LOS FENOMENOS OPTOELECTRONICOS EN MICROCAVIDADES/
info:eu-repo/grantAgreement/MINECO//MAT2015-69669-P/ES/OPTOLECTRONICA EN NANOCAVIDADES DE ALTO INDICE DE REFRACCION. DEL SILICIO A LA PEROVSKITA/
info:eu-repo/grantAgreement/MINECO//TEC2015-74405-JIN/ES/MICRO- Y NANO-CAVIDADES BASADAS EN PEROVSKITA HALOGENADA. CELULAS SOLARES Y EMISORES DE LUZ/
info:eu-repo/grantAgreement/MINECO//ENE2013-49984-EXP/ES/SUPERANDO EL CUERPO NEGRO. ABSORCION Y EMISION DE LUZ EN UNA MICROESFERA DE SILICIO./
info:eu-repo/grantAgreement/MINECO//ENE2015-74009-JIN/ES/HACIA LA OBTENCION DE MULTIPLES CELULAS MONOCRISTALINAS DE SILICIO CON 20% DE EFICIENCIA Y MENOS DE 20 µM DE GROSOR A PARTIR DE UNA UNICA OBLEA./
info:eu-repo/grantAgreement/MINECO//SEV-2016-0683/
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Agradecimientos:
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This work was supported by several projects of the Spanish Ministry of Economy and Competitiveness (MINECO), Severo Ochoa program for Centers of Excellence (SEV-2016-0683), MAT2015-69669-PM, ENE2013-49984-EXP, ENE2015-74009-JIN ...[+]
This work was supported by several projects of the Spanish Ministry of Economy and Competitiveness (MINECO), Severo Ochoa program for Centers of Excellence (SEV-2016-0683), MAT2015-69669-PM, ENE2013-49984-EXP, ENE2015-74009-JIN (cofunded by the European Regional Development Fund), and of the Spanish Science, Innovation and Universities, PGC2018-099744-B-100. F.R.-M. thanks the financial contribution of MINECO through the program for young researchers support, TEC 2015 2015-74405-JIN. The authors greatly acknowledge the contribution of Prof. Francisco Meseguer for both the fruitful discussions and the revision of the manuscript, and Prof. Marie Louise McCarrey for careful proofreading of the manuscript.
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Tipo:
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Artículo
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