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dc.creatorNarvaez, Gustavo A.
dc.creatorKim, Jeongnim
dc.creatorWilkins, John W.
dc.date.accessioned2011-03-03T17:26:22Z
dc.date.available2011-03-03T17:26:22Z
dc.date.issued2005-10-14
dc.identifier.citationGustavo A. Narvaez, Jeongnim Kim, John W. Wilkins, "Effects of morphology on phonons in nanoscopic silver grains," Physical Review B 72, no. 15 (2005), doi:10.1103/PhysRevB.72.155411en_US
dc.identifier.issn1550-235X
dc.identifier.urihttp://hdl.handle.net/1811/48112
dc.description.abstractThe morphology of nanoscopic Ag grains significantly affects the phonons. Atomistic simulations show that realistic nanograin models display complex vibrational properties. (1) Single-crystalline grains. Nearly pure torsional and radial phonons appear at low frequencies. For low-energy, faceted models, the breathing mode and acoustic gap (lowest frequency) are about 10% lower than predicted by elasticity theory (ET) for a continuum sphere of the same volume. The sharp edges and the atomic lattice split the ET-acoustic-gap quintet into a doublet and triplet. The surface protrusions associated with nearly spherical, high-energy models produce a smaller acoustic gap and a higher vibrational density of states (DOS) at frequencies ν<2 THz. (2) Twined icosahedra. In contrast to the single-crystal case, the inherent strain produce a larger acoustic gap, while the core atoms yield a DOS tail extending beyond the highest frequency of single-crystalline grains. (3) Mark's decahedra, in contrast to (1) and (2), do not have a breathing mode; although twined and strained, do not exhibit a high-frequency tail in the DOS. (4) Irregular nanograins. Grain boundaries and surface disorder yield nondegenerate phonon frequencies, and significantly smaller acoustic gap. Only these nanograins exhibit a low-frequency ν^2 DOS in the interval 1–2 THz.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Physical Societyen_US
dc.rights©2005 The American Physical Societyen_US
dc.titleEffects of morphology on phonons in nanoscopic silver grainsen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevB.72.155411
dc.identifier.osuauthorwilkins.5


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