2018
DOI: 10.1039/c7qi00822h
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The stability of hollow nanoparticles and the simulation temperature ramp

Abstract: Hollow nanoparticles (hNPs) are of interest because their large cavities and small thickness give rise to a large surface to volume ratio.

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Cited by 10 publications
(30 citation statements)
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“…This criterion was chosen based on Cao et al 21 findings, which show a strong surface reorientation when the NT thickness is close to 1 nm. We note that this behavior has also been observed in other hollow structures 49 51 , for a specific combination of radius and thickness. In those cases, the surface stress is not compensated by the shell, originating a partial shrinkage, and the surface reorientation is assisted by Shockley partial dislocations as the dominant mechanism.…”
Section: Methodssupporting
confidence: 79%
“…This criterion was chosen based on Cao et al 21 findings, which show a strong surface reorientation when the NT thickness is close to 1 nm. We note that this behavior has also been observed in other hollow structures 49 51 , for a specific combination of radius and thickness. In those cases, the surface stress is not compensated by the shell, originating a partial shrinkage, and the surface reorientation is assisted by Shockley partial dislocations as the dominant mechanism.…”
Section: Methodssupporting
confidence: 79%
“…On the one hand, excess energy due to the grain boundary structure can trigger the grain boundary sliding and the shrinkage of the NS [48]. On the other hand, while typical Au hollow nanospheres with thicknesses of 5 nm and diameters of 50 nm are stable at room temperature [52][53][54], the porous structure of the NS increases the surface area, which can drive the collapse of the nanostructure due to surface stresses [48]. Therefore, we adopted a relaxation time of 10 ns using a timestep of 1.0 fs at 400 K. Then, the system temperature was cooled to 300 K, in 0.1 ps with a time step of 1.0 fs.…”
Section: Methodsmentioning
confidence: 99%
“…Las W-hNPs fueron construidas a partir de <100> W, seleccionando dos esferas concéntricas de 5,0 y 7,5 nm de radio, obteniendo como resultado una W-hNP completamente cristalina, con un radio externo de 7,5 nm y un espesor de 2,5 nm (detallada en la Figura 7.1). Este proceso ha sido empleado en otras ocasiones para analizar la estabilidad de W-hNPs, confirmándose los resultados obtenidos con medidas experimentales [85,243,244]. Las W-hNPs simuladas siguieron un proceso de relajación por calentamiento para eliminar tensiones residuales [243].…”
Section: Simulaciones Atomísticasunclassified
“…Este proceso ha sido empleado en otras ocasiones para analizar la estabilidad de W-hNPs, confirmándose los resultados obtenidos con medidas experimentales [85,243,244]. Las W-hNPs simuladas siguieron un proceso de relajación por calentamiento para eliminar tensiones residuales [243]. El estudio de la estabilidad térmica se llevó a cabo aumentando la temperatura de la W-hNP diseñada desde un valor inicial de 300 K hasta alcanzar 3000 K en pasos de 20 K cada 0,2 ns, empleando para ello un termostato Noose-Hoover con un paso de tiempo de 1 fs.…”
Section: Simulaciones Atomísticasunclassified
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