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j.ijsolstr.2009.05.018.pdf1.19 MBAdobe PDF見る/開く
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dc.contributor.authorZhang, J.Y.en
dc.contributor.authorGuest, S.D.en
dc.contributor.authorConnelly, R.en
dc.contributor.authorOhsaki, M.en
dc.contributor.alternative張, 景耀ja
dc.contributor.alternative大﨑, 純ja
dc.date.accessioned2023-02-20T09:15:29Z-
dc.date.available2023-02-20T09:15:29Z-
dc.date.issued2010-01-01-
dc.identifier.urihttp://hdl.handle.net/2433/279337-
dc.description.abstractThis paper presents conditions for self-equilibrium and super stability of dihedral ‘star’ tensegrity structures, based on their dihedral symmetry. It is demonstrated that the structures are super stable if and only if they have an odd number of struts, and the struts are as close as possible to each other. Numerical investigations show that their prestress stability is sensitive to the geometry realisation.en
dc.language.isoeng-
dc.publisherElsevier BVen
dc.rights© 2010. This manuscript version is made available under the CC-BY-NC-ND 4.0 license.en
dc.rightsThe full-text file will be made open to the public on 1 January 2012 in accordance with publisher's 'Terms and Conditions for Self-Archiving'.en
dc.rightsThis is not the published version. Please cite only the published version. この論文は出版社版でありません。引用の際には出版社版をご確認ご利用ください。en
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectTensegrity structureen
dc.subjectDihedral symmetryen
dc.subjectBlock-diagonalisationen
dc.subjectSelf-equilibriumen
dc.subjectStabilityen
dc.titleDihedral ‘star’ tensegrity structuresen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleInternational Journal of Solids and Structuresen
dc.identifier.volume47-
dc.identifier.issue1-
dc.identifier.spage1-
dc.identifier.epage9-
dc.relation.doi10.1016/j.ijsolstr.2009.05.018-
dc.textversionauthor-
dcterms.accessRightsopen access-
datacite.date.available2012-01-01-
dc.identifier.pissn0020-7683-
dc.identifier.eissn1879-2146-
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