Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9314
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dc.contributor.authorallViolay, M. E. S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallNielsen, S. B.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallGibert, B.; Géosciences Montpellier UMR5243, Université Montpellier, 2 Place Bataillon, 34095 Montpellier cedex 5, Franceen
dc.contributor.authorallSpagnuolo, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallCavallo, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallAzais, P.; Géosciences Montpellier UMR5243, Université Montpellier, 2 Place Bataillon, 34095 Montpellier cedex 5, Franceen
dc.contributor.authorallVinciguerra, S.; Dipartimento di Scienze della Terra, Università degli Studi di Torino, Via Valperga Caluso 35, 10125 Turin, Italyen
dc.contributor.authorallDi Toro, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.date.accessioned2015-02-09T07:52:28Zen
dc.date.available2015-02-09T07:52:28Zen
dc.date.issued2013-12en
dc.identifier.urihttp://hdl.handle.net/2122/9314en
dc.description.abstractFluid-rock interactions can control earthquake nucleation and the evolution of earthquake sequences. Experimental studies of fault frictional properties in the presence of fl uid can provide unique insights into these interactions. We report the fi rst results from experiments performed on cohesive silicate-bearing rocks (microgabbro) in the presence of pressurized pore fl uids (H2 O, drained conditions) at realistic seismic deformation conditions. The experimental data are compared with those recently obtained from carbonate-bearing rocks (Carrara marble). Contrary to theoretical arguments, and consistent with the interpretation of some fi eld observations, we show that frictional melting of a microgabbro develops in the presence of water. In microgabbro, the initial weakening mechanism (fl ash melting of the asperities) is delayed in the presence of water; conversely, in calcite marble the weakening mechanism (brittle failure of the asperities) is favored. This opposite behavior highlights the importance of host-rock composition in controlling dynamic (frictional) weakening in the presence of water: cohesive carbonate-bearing rocks are more prone to slip in the presence of water, whereas the presence of water might delay or inhibit the rupture nucleation and propagation in cohesive silicate-bearing rocks.en
dc.language.isoEnglishen
dc.publisher.nameGeological Society of Americaen
dc.relation.ispartofGeology (Geological Society of America)en
dc.relation.ispartofseries1/42 (2013)en
dc.subjectcarbonates faultsen
dc.subjecthydro-elasto-dynamicsen
dc.subjectearthquake nucleationen
dc.subjectfrictionen
dc.subjectrock mechanicsen
dc.subjectfluid-rcok interactionsen
dc.titleEffect of water on the frictional behavior of cohesive rocks during earthquakesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber27-30en
dc.subject.INGV03. Hydrosphere::03.04. Chemical and biological::03.04.06. Hydrothermal systemsen
dc.subject.INGV04. Solid Earth::04.01. Earth Interior::04.01.04. Mineral physics and properties of rocksen
dc.subject.INGV04. Solid Earth::04.01. Earth Interior::04.01.05. Rheologyen
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.06. Rheology, friction, and structure of fault zonesen
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.01. Earthquake faults: properties and evolutionen
dc.identifier.doi10.1130/G34916.1en
dc.description.obiettivoSpecifico4T. Fisica dei terremoti e scenari cosismicien
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.relation.issn0091-7613en
dc.relation.eissn1943-2682en
dc.contributor.authorViolay, M. E. S.en
dc.contributor.authorNielsen, S. B.en
dc.contributor.authorGibert, B.en
dc.contributor.authorSpagnuolo, E.en
dc.contributor.authorCavallo, A.en
dc.contributor.authorAzais, P.en
dc.contributor.authorVinciguerra, S.en
dc.contributor.authorDi Toro, G.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentGéosciences Montpellier UMR5243, Université Montpellier, 2 Place Bataillon, 34095 Montpellier cedex 5, Franceen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentGéosciences Montpellier UMR5243, Université Montpellier, 2 Place Bataillon, 34095 Montpellier cedex 5, Franceen
dc.contributor.departmentDipartimento di Scienze della Terra, Università degli Studi di Torino, Via Valperga Caluso 35, 10125 Turin, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextreserved-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptEPFL, LEMR, Lausanne, Switzerland-
crisitem.author.deptDurham University, Durham, UK-
crisitem.author.deptGéosciences Montpellier UMR5243, Université Montpellier, 2 Place Bataillon, 34095 Montpellier cedex 5, France-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptGéosciences Montpellier UMR5243, Université Montpellier, 2 Place Bataillon, 34095 Montpellier cedex 5, France-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0002-7402-8263-
crisitem.author.orcid0000-0002-9214-2932-
crisitem.author.orcid0000-0002-1377-5812-
crisitem.author.orcid0000-0002-6939-3549-
crisitem.author.orcid0000-0002-6618-3474-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent03. Hydrosphere-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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