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dc.contributor.authorMurakami, M.
dc.contributor.authorKohara, S
dc.contributor.authorKitamura, N.
dc.contributor.authorAkola, Jaakko
dc.contributor.authorInoue, H
dc.contributor.authorHirata, A
dc.contributor.authorHiraoka, Y
dc.contributor.authorOnodera, Y
dc.contributor.authorObayashi, I
dc.contributor.authorKalikka, J
dc.contributor.authorHirao, N
dc.contributor.authorMusso, T
dc.contributor.authorFoster, Adam S
dc.contributor.authorIdemoto, Y
dc.contributor.authorSakata, O
dc.contributor.authorOhishi, Y
dc.date.accessioned2020-04-07T07:28:16Z
dc.date.available2020-04-07T07:28:16Z
dc.date.created2019-11-06T16:26:42Z
dc.date.issued2019
dc.identifier.issn2469-9950
dc.identifier.urihttps://hdl.handle.net/11250/2650573
dc.description.abstractHigh-pressure synthesis of denser glass has been a longstanding interest in condensed-matter physics and materials science because of its potentially broad industrial application. Nevertheless, understanding its nature under extreme pressures has yet to be clarified due to experimental and theoretical challenges. Here we reveal the formation of OSi4 tetraclusters associated with that of SiO7 polyhedra in SiO2 glass under ultrahigh pressures to 200 gigapascal confirmed both experimentally and theoretically. Persistent homology analyses with molecular dynamics simulations found increased packing fraction of atoms whose topological diagram at ultrahigh pressures is similar to a pyrite-type crystalline phase, although the formation of tetraclusters is prohibited in the crystalline phase. This critical difference would be caused by the potential structural tolerance in the glass for distortion of oxygen clusters. Furthermore, an expanded electronic band gap demonstrates that chemical bonds survive at ultrahigh pressure. This opens up the synthesis of topologically disordered dense oxide glassesen_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.titleUltrahigh-pressure form of Si O2 glass with dense pyrite-type crystalline homologyen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.source.volume99en_US
dc.source.journalPhysical review B (PRB)en_US
dc.source.issue4en_US
dc.identifier.doi10.1103/PhysRevB.99.045153
dc.identifier.cristin1744687
dc.description.localcode© American Physical Society 2019.en_US
cristin.unitcode194,66,20,0
cristin.unitnameInstitutt for fysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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