2015
DOI: 10.1134/s0031918x15040055
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Analysis of the heat capacity of nanoclusters of FCC metals on the example of Al, Ni, Cu, Pd, and Au

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Cited by 23 publications
(18 citation statements)
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“…Given the vast number of possible configurations to assess, a pure DFT approach is not tractable. For the Cu–Cu interatomic interactions, we have chosen to use the Gupta many-body potentials by Cleri and Rosato, which have been widely used in a study of cluster structures, their growth and dynamics, and, in particular, in the structure prediction of Cu n clusters ( n ≤ 56) using a genetic algorithm (GA) …”
Section: Resultsmentioning
confidence: 99%
“…Given the vast number of possible configurations to assess, a pure DFT approach is not tractable. For the Cu–Cu interatomic interactions, we have chosen to use the Gupta many-body potentials by Cleri and Rosato, which have been widely used in a study of cluster structures, their growth and dynamics, and, in particular, in the structure prediction of Cu n clusters ( n ≤ 56) using a genetic algorithm (GA) …”
Section: Resultsmentioning
confidence: 99%
“…The structural and static properties of Au N clusters and nanoparticles have been widely investigated, and some of the works provide an explicit comparison between the data from calculated structures (mostly in the DFT framework) and experimental data. However, although the early experiment of Buffat and Borel was concerned with gold nanoparticles, no experimental size-selected determination of the caloric curves in the cluster regime range ( N less than 50) has been published so far to our knowledge. A number of theoretical investigations usually achieved with many-body potentials or thermodynamical models have examined thermodynamically induced structural conversion and the melting of large nanoparticles. Simulations of the thermal properties were also carried out in the cluster regime size (from one to a few tens).…”
Section: Introductionmentioning
confidence: 99%
“…The steady-state temperature of the sample surface increases from 52 °C for bare BiCuSeO to 55 °C for 4-nm-thick AuNP layer/BiCuSeO and 58 °C for 7-nm-thick AuNP layer/BiCuSeO. This is probably due to the fact that the heat capacity C p of AuNPs (27 Jmol −1 K −1 ) is much smaller than that of BiCuSeO (99.5 Jmol −1 K −1 ), leading to a higher temperature rise when absorbing a similar amount of light energy [29, 30]. In addition, the introduction of the amorphous AuNP layer may reduce the reflectance loss of light at the smooth BiCuSeO film surface.…”
Section: Resultsmentioning
confidence: 99%