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dc.contributor.authorFan, Chia-Chengen_US
dc.contributor.authorFang, Yung-Showen_US
dc.date.accessioned2019-04-02T05:59:42Z-
dc.date.available2019-04-02T05:59:42Z-
dc.date.issued2010-11-01en_US
dc.identifier.issn0266-352Xen_US
dc.identifier.urihttp://dx.doi.org/10.1016/j.compgeo.2010.08.004en_US
dc.identifier.urihttp://hdl.handle.net/11536/150202-
dc.description.abstractFor retaining walls built in mountainous regions, narrow backfill spaces are often encountered. The space to fully develop the active wedge is restricted for walls with a limited backfill space. This paper presents a numerical study on the behaviour of active earth pressures behind a rigid retaining wall with limited backfill space of various geometries. The active earth pressure for a wall built with limited backfill space is considerably less than that of the Coulomb solution, and the location of the resultant of active earth pressures is noticeably higher than one-third of the wall height. The coefficient of active earth pressures is as low as 0.5-0.6 times the Coulomb solution and the h/H value reaches up to 0.4-0.37 if aspect ratio of the fill space is in the range from 0.1 to 0.2. A clear trend between the ratio of the coefficient of active earth pressures at constrained fill conditions over the Coulomb K(a) value and the aspect ratio of the fill-space geometry is obtained. (C) 2010 Elsevier Ltd. All rights reserved.en_US
dc.language.isoen_USen_US
dc.subjectActive earth pressureen_US
dc.subjectLimited backfill spaceen_US
dc.subjectFinite element analysisen_US
dc.subjectAspect ratioen_US
dc.titleNumerical solution of active earth pressures on rigid retaining walls built near rock facesen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.compgeo.2010.08.004en_US
dc.identifier.journalCOMPUTERS AND GEOTECHNICSen_US
dc.citation.volume37en_US
dc.citation.spage1023en_US
dc.citation.epage1029en_US
dc.contributor.department土木工程學系zh_TW
dc.contributor.departmentDepartment of Civil Engineeringen_US
dc.identifier.wosnumberWOS:000285220300021en_US
dc.citation.woscount17en_US
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