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Article: Morphology of nested fullerenes

TitleMorphology of nested fullerenes
Authors
Issue Date1995
Citation
Physical Review Letters, 1995, v. 74, n. 10, p. 1779-1782 How to Cite?
AbstractWe introduce a continuum model which shows that dislocations and/or grain boundaries are intrinsic features of nested fullerenes whose thickness exceeds a critical value to relieve the large inherent strains in these structures. The ratio of the thickness to the radius of the nested fullerenes is determined by the ratio of the surface to curvature and dislocation (or grain boundary) energies. Confirming experimental evidence is presented for nested fullerenes with small thicknesses and with spherosymmetric shapes. © 1995 The American Physical Society.
Persistent Identifierhttp://hdl.handle.net/10722/303791
ISSN
2021 Impact Factor: 9.185
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ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorSrolovitz, D. J.-
dc.contributor.authorSafran, S. A.-
dc.contributor.authorHomyonfer, M.-
dc.contributor.authorTenne, R.-
dc.date.accessioned2021-09-15T08:26:01Z-
dc.date.available2021-09-15T08:26:01Z-
dc.date.issued1995-
dc.identifier.citationPhysical Review Letters, 1995, v. 74, n. 10, p. 1779-1782-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10722/303791-
dc.description.abstractWe introduce a continuum model which shows that dislocations and/or grain boundaries are intrinsic features of nested fullerenes whose thickness exceeds a critical value to relieve the large inherent strains in these structures. The ratio of the thickness to the radius of the nested fullerenes is determined by the ratio of the surface to curvature and dislocation (or grain boundary) energies. Confirming experimental evidence is presented for nested fullerenes with small thicknesses and with spherosymmetric shapes. © 1995 The American Physical Society.-
dc.languageeng-
dc.relation.ispartofPhysical Review Letters-
dc.titleMorphology of nested fullerenes-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1103/PhysRevLett.74.1779-
dc.identifier.scopuseid_2-s2.0-0000618091-
dc.identifier.volume74-
dc.identifier.issue10-
dc.identifier.spage1779-
dc.identifier.epage1782-
dc.identifier.isiWOS:A1995QK07500021-

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