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Ideally, those clusters do not overlap.
Since GDD does not require any special parameters prior to run, resulting clusters do not change at different runs.
These results serve as the first indication that Fe2 clusters do not agglomerate during the pyrolysis process.
Moreover, galactic clusters do not appear to have enough mass in them to stop themselves flying apart.
The majority of compact binaries which formed from the population of primordial binaries in young and dense star clusters do not lead to detectable gravitational wave sources.
In situ electrochemical analysis shows that the incorporated PW clusters do not affect material activity, however they do play a role in defining both meso- and micro-structure.
However, current approaches and designs for OpenSHMEM on GPU clusters do not take advantage of the GDR features leading to potential performance improvements being untapped.
Ag nanoparticles greatly promote the reduction and catalytic activity in CO oxidation of CeO2 nanocrystals but positively charged Ag+n clusters do not.
In the large-scale group decision making (LGDM) consensus process, it is usually assumed that the obtained clusters do not change.
Larger clusters do not carry enough energy per atom to cause such effects and their energy is dissipated in the substrate as heat.
The diameters of the adsorbed clusters increase with time and the cathodic polarization, while the heights of the adsorbed clusters do not increase obviously.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com