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dc.contributor.authorGómez Frutos, Daniel
dc.contributor.authorCastro Dorado, Antonio
dc.contributor.authorGutiérrez Alonso, Gabriel
dc.date.accessioned2023-05-29T08:25:06Z
dc.date.available2023-05-29T08:25:06Z
dc.date.issued2023-01-11
dc.identifier.citationD. Gómez-Frutos, A. Castro and G. Gutiérrez-Alonso. Post-collisional batholiths do contribute to continental growth. Earth and Planetary Science Letters 603 (2023) 117978. [https://doi.org/10.1016/j.epsl.2022.117978]es_ES
dc.identifier.urihttps://hdl.handle.net/10481/81899
dc.descriptionThis work was supported through the Spanish Research Agency (AEI) Grant N◦ PGC2018-096534-B-I00 (Proyecto IBERCRUST). We acknowledge the support received from the Instituto Andaluz de Ciencias de la Tierra (CSIC - UGR) and its staff for the installa- tion of a high-pressure laboratory. We are particularly grateful to Taras Gerya and Mike Fowler for their positive and constructive feedback. We also want to thank Rosemary Hickey-Vargas for her handling of this manuscript.es_ES
dc.descriptionSupplementary material related to this article can be found on- line at https://doi.org/10.1016/j.epsl.2022.117978es_ES
dc.description.abstractPost-collisional voluminous silicic magmatism is represented in most orogens across the world in the form of large granodiorite batholiths and minor intermediate and mafic intrusions, postdating 5-30 Ma the age of the collisional paroxysm responsible of the main mountain building events. Post-collisional mafic intrusions are acknowledged as a mechanism that contributes to long-term yet minor continental growth. The silicic magmas forming the large batholiths, however, have been dismissed from the crustal growth discussion due to bias in the conception that they always generate by recycling older lower crustal igneous rocks. Contrary to this, geochemical and isotopic relations together with new experimental data provided in this paper suggest that the post-collisional signature can be reproduced without the implication of a crustal component, supporting a potential common origin for the two suites, intermediate and silicic. That is, both suites can be derived from a metasomatized mantle source, thus representing the injection of largely juvenile material to produce new continental crust. This inference is contextualized within the supercontinent cycle, showing that the timing of post-collisional magmatism accounts for the generation and preservation rates predicted by the existing models, since both reach maximum values in the amalgamation-collisional stage of the supercontinent cycle, rather than in the subduction stage. All together these inferences lead to think that post-Archean, post-collisional magmatism has been significantly underestimated when computing continental crustal growth through time.es_ES
dc.description.sponsorshipSpanish Government PGC2018-096534-B-I00es_ES
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectCrustal growthes_ES
dc.subjectContinental crustes_ES
dc.subjectPost-collisional magmatismes_ES
dc.subjectMetasomatized mantlees_ES
dc.subjectTectonicses_ES
dc.subjectBatholithes_ES
dc.titlePost-collisional batholiths do contribute to continental growthes_ES
dc.typejournal articlees_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1016/j.epsl.2022.117978
dc.type.hasVersionVoRes_ES


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