Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors
- Autores
- Gardey Merino, María
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión aceptada
- Descripción
- Solar selective paints, with the addition of Co3O4 as a pigment, are used to improve energetic efficiency in solar collectors. Although Co3O4 has been obtained by different methods, references about combustion synthesis are scarce. Co3O4 powders have been synthesized by stoichiometric and non-stoichiometric routes using aspartic acid (Asp) or tri-hydroxi-methyl-aminomethane (Tris) as fuels. The samples were calcined in air at 500 °C. They were characterized by X-ray diffraction, scanning electron microscopy, transmission electron microscopy, thermogravimetric analysis, differential scanning calorimetry, Fourier transform infrared spectrum and the specific surface area of the samples was determined by means of the Brunauer–Emmett–Teller technique. The optical properties of pigments were assessed by means of a spectrophotometer. In all cases, powders exhibited the crystalline structure of Co3O4. A minimum crystallite average size of 29 nm was observed for powders obtained by the “stoichiometric/Asp” combustion route, while a maximum value of 41 nm was stated for powders obtained by the “nonstoichiometric/Asp” combustion process. The average particle size ranged between 50 and 100 nm. The powders obtained by the “stoichiometric/Asp” method were selected to study their optical properties; their solar absorption value was 86%. Solar selective surfaces composed by Co3O4 pigments and an alkyd resin were obtained and applied over copper or aluminum substrates. In both cases, solar absorptance was of 93% and comparable with similar solar selective surfaces, but the thermal emittance value was higher than 90%, as a consequence of the large width of the films.
Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza; Argentina
Peer Reviewed - Fuente
- Procedia Materials Science 9 , 230 – 238. ( 2015 )
- Materia
- Cobalt oxide nanoparticles, Gel combustion-process, Solar absorptance, Optical spectroscopy, X-ray diffraction
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- 2023-12-18T14:47:43Z
- Repositorio
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- Institución
- Universidad Tecnológica Nacional
- OAI Identificador
- oai:ria.utn.edu.ar:20.500.12272/9251
Ver los metadatos del registro completo
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Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectorsGardey Merino, MaríaCobalt oxide nanoparticles, Gel combustion-process, Solar absorptance, Optical spectroscopy, X-ray diffractionSolar selective paints, with the addition of Co3O4 as a pigment, are used to improve energetic efficiency in solar collectors. Although Co3O4 has been obtained by different methods, references about combustion synthesis are scarce. Co3O4 powders have been synthesized by stoichiometric and non-stoichiometric routes using aspartic acid (Asp) or tri-hydroxi-methyl-aminomethane (Tris) as fuels. The samples were calcined in air at 500 °C. They were characterized by X-ray diffraction, scanning electron microscopy, transmission electron microscopy, thermogravimetric analysis, differential scanning calorimetry, Fourier transform infrared spectrum and the specific surface area of the samples was determined by means of the Brunauer–Emmett–Teller technique. The optical properties of pigments were assessed by means of a spectrophotometer. In all cases, powders exhibited the crystalline structure of Co3O4. A minimum crystallite average size of 29 nm was observed for powders obtained by the “stoichiometric/Asp” combustion route, while a maximum value of 41 nm was stated for powders obtained by the “nonstoichiometric/Asp” combustion process. The average particle size ranged between 50 and 100 nm. The powders obtained by the “stoichiometric/Asp” method were selected to study their optical properties; their solar absorption value was 86%. Solar selective surfaces composed by Co3O4 pigments and an alkyd resin were obtained and applied over copper or aluminum substrates. In both cases, solar absorptance was of 93% and comparable with similar solar selective surfaces, but the thermal emittance value was higher than 90%, as a consequence of the large width of the films.Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza; ArgentinaPeer Reviewed2023-12-18T14:47:43Z2023-12-18T14:47:43Z2015-01-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloplainapplication/pdfProcedia Materials Sciencehttp://hdl.handle.net/20.500.12272/925110.1016/j.mspro.2015.04.029Procedia Materials Science 9 , 230 – 238. ( 2015 )reponame:Repositorio Institucional Abierto (UTN)instname:Universidad Tecnológica Nacionalengenginfo:eu-repo/semantics/openAccess2023-12-18T14:47:43Zhttp://creativecommons.org/publicdomain/zero/1.0/CC0 1.0 UniversalUniversidad Tecnológica Nacional. Facultad Regional MendozaAtribución2026-09-24T12:45:13Zoai:ria.utn.edu.ar:20.500.12272/9251instacron:UTNInstitucionalhttp://ria.utn.edu.ar/Universidad públicaNo correspondehttp://ria.utn.edu.ar/oaigestionria@rec.utn.edu.ar; fsuarez@rec.utn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:a2026-09-24 12:45:14.355Repositorio Institucional Abierto (UTN) - Universidad Tecnológica Nacionalfalse |
| dc.title.none.fl_str_mv |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| title |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| spellingShingle |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors Gardey Merino, María Cobalt oxide nanoparticles, Gel combustion-process, Solar absorptance, Optical spectroscopy, X-ray diffraction |
| title_short |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| title_full |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| title_fullStr |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| title_full_unstemmed |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| title_sort |
Combustion synthesis of ultrafine powders of Co3O4 for selective surfaces of solar collectors |
| dc.creator.none.fl_str_mv |
Gardey Merino, María |
| author |
Gardey Merino, María |
| author_facet |
Gardey Merino, María |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Cobalt oxide nanoparticles, Gel combustion-process, Solar absorptance, Optical spectroscopy, X-ray diffraction |
| topic |
Cobalt oxide nanoparticles, Gel combustion-process, Solar absorptance, Optical spectroscopy, X-ray diffraction |
| dc.description.none.fl_txt_mv |
Solar selective paints, with the addition of Co3O4 as a pigment, are used to improve energetic efficiency in solar collectors. Although Co3O4 has been obtained by different methods, references about combustion synthesis are scarce. Co3O4 powders have been synthesized by stoichiometric and non-stoichiometric routes using aspartic acid (Asp) or tri-hydroxi-methyl-aminomethane (Tris) as fuels. The samples were calcined in air at 500 °C. They were characterized by X-ray diffraction, scanning electron microscopy, transmission electron microscopy, thermogravimetric analysis, differential scanning calorimetry, Fourier transform infrared spectrum and the specific surface area of the samples was determined by means of the Brunauer–Emmett–Teller technique. The optical properties of pigments were assessed by means of a spectrophotometer. In all cases, powders exhibited the crystalline structure of Co3O4. A minimum crystallite average size of 29 nm was observed for powders obtained by the “stoichiometric/Asp” combustion route, while a maximum value of 41 nm was stated for powders obtained by the “nonstoichiometric/Asp” combustion process. The average particle size ranged between 50 and 100 nm. The powders obtained by the “stoichiometric/Asp” method were selected to study their optical properties; their solar absorption value was 86%. Solar selective surfaces composed by Co3O4 pigments and an alkyd resin were obtained and applied over copper or aluminum substrates. In both cases, solar absorptance was of 93% and comparable with similar solar selective surfaces, but the thermal emittance value was higher than 90%, as a consequence of the large width of the films. Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza; Argentina Peer Reviewed |
| description |
Solar selective paints, with the addition of Co3O4 as a pigment, are used to improve energetic efficiency in solar collectors. Although Co3O4 has been obtained by different methods, references about combustion synthesis are scarce. Co3O4 powders have been synthesized by stoichiometric and non-stoichiometric routes using aspartic acid (Asp) or tri-hydroxi-methyl-aminomethane (Tris) as fuels. The samples were calcined in air at 500 °C. They were characterized by X-ray diffraction, scanning electron microscopy, transmission electron microscopy, thermogravimetric analysis, differential scanning calorimetry, Fourier transform infrared spectrum and the specific surface area of the samples was determined by means of the Brunauer–Emmett–Teller technique. The optical properties of pigments were assessed by means of a spectrophotometer. In all cases, powders exhibited the crystalline structure of Co3O4. A minimum crystallite average size of 29 nm was observed for powders obtained by the “stoichiometric/Asp” combustion route, while a maximum value of 41 nm was stated for powders obtained by the “nonstoichiometric/Asp” combustion process. The average particle size ranged between 50 and 100 nm. The powders obtained by the “stoichiometric/Asp” method were selected to study their optical properties; their solar absorption value was 86%. Solar selective surfaces composed by Co3O4 pigments and an alkyd resin were obtained and applied over copper or aluminum substrates. In both cases, solar absorptance was of 93% and comparable with similar solar selective surfaces, but the thermal emittance value was higher than 90%, as a consequence of the large width of the films. |
| publishDate |
2015 |
| dc.date.none.fl_str_mv |
2015-01-01 2023-12-18T14:47:43Z 2023-12-18T14:47:43Z |
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info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
acceptedVersion |
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Procedia Materials Science http://hdl.handle.net/20.500.12272/9251 10.1016/j.mspro.2015.04.029 |
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Procedia Materials Science 10.1016/j.mspro.2015.04.029 |
| url |
http://hdl.handle.net/20.500.12272/9251 |
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eng eng |
| language |
eng |
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openAccess |
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2023-12-18T14:47:43Z http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal Universidad Tecnológica Nacional. Facultad Regional Mendoza Atribución |
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plain application/pdf |
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Repositorio Institucional Abierto (UTN) - Universidad Tecnológica Nacional |
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