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Probing radiation resistance in simulated metallic core–shell nanoparticles

cnea.tipodocumentoARTÍCULO CIENTÍFICO
dc.contributor.authorTramontina Videla, Diego Ramiro
dc.contributor.authorDeluigi, Orlando Raul
dc.contributor.authorPinzón, R.
dc.contributor.authorRojas Nunez, J.
dc.contributor.authorValencia, F. J.
dc.contributor.authorPasianot, Roberto Cesar
dc.contributor.authorBaltazar, S. E.
dc.contributor.authorGonzalez, R. I.
dc.contributor.authorBringa, Eduardo Marcial
dc.date.accessioned2025-12-11T23:31:43Z
dc.date.available2025-12-11T23:31:43Z
dc.date.issued2023-08
dc.description.abstractWe present molecular dynamics (MD) simulations of radiation damage in Fe nanoparticles (NP) and bimetallic FeCu core–shell nanoparticles (CSNP). The CSNP includes a perfect body-centered cubic (bcc) Fe core coated with a face-centered cubic (fcc) Cu shell. Irradiation with Fe Primary Knock-on Atoms (PKA) with energies between 1 and 7 keV leads to point defects, without clustering beyond divacancies and very few slightly larger vacancy clusters, and without interstitial clusters, unlike what happens in bulk at the same PKA energies. The Fe-Cu interface and shell can act as a defect sink, absorbing radiation-induced damage and, therefore, the final number of defects in the Fe core is significantly lower than in the Fe NP. In addition, the Cu shell substantially diminishes the number of sputtered Fe atoms, acting as a barrier for recoil ejection. Structurally, the Cu shell responds to the stress generated by the collision cascade by creating and destroying stacking faults across the shell width, which could also accommodate further irradiation defects. We compare our MD results to Monte Carlo Binary Collision Approximation (BCA) simulations using the SRIM code, for the irradiation of an amorphous 3-layer thin film with a thickness equal to the CSNP diameter. BCA does not include defect recombination, so the number of Frenkel pairs is significantly higher than in MD, as expected. Sputtering yield (Y) is underestimated by BCA, which is also expected since the simulation is for a thin film at normal incidence. We also compare MD defect production to bulk predictions of the analytic Athermal Recombination Corrected Displacements Per Atom (arc-dpa) model. The number of vacancies in the Fe core is only slightly lower than arc-dpa predictions, but the number of interstitials is reduced by about one order of magnitude compared to vacancies, at 5 keV. According to the radiation resistance found for FeCu CSNP in our simulations, this class of nanomaterial could be suitable for developing new radiation-resistant coatings, nanostructured components, and shields for use in extreme environments, for instance, in nuclear energy and astrophysical applications.
dc.description.institutionalaffiliationFil: Tramontina Videla, Diego Ramiro. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina. Universidad de Mendoza; Argentina
dc.description.institutionalaffiliationFil: Deluigi, Orlando Raul. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina. Universidad de Mendoza; Argentina
dc.description.institutionalaffiliationFil: Pinzón, R.. Universidad Tecnologica de Panamá.; Panamá. Sistema Nacional de Investigación; Panamá. Centro de Estudios Multidisciplinarios de Ingeniería Ciencias y Tecnología; Panamá
dc.description.institutionalaffiliationFil: Rojas Nunez, J.. Universidad de Santiago de Chile; Chile. Center for the Development of Nanoscience and Nanotechnology; Chile
dc.description.institutionalaffiliationFil: Valencia, F. J.. Center For Development Of Nanoscience And Technology; Chile. Universidad Católica de Maule; Chile
dc.description.institutionalaffiliationFil: Pasianot, Roberto Cesar. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Gerencia de Área de Energía Nuclear. Gerencia Materiales; Argentina. Universidad Nacional de San Martín. Instituto Sabato; Argentina
dc.description.institutionalaffiliationFil: Baltazar, S. E.. Universidad de Santiago de Chile; Chile. Center For Development Of Nanoscience And Technology; Chile
dc.description.institutionalaffiliationFil: Gonzalez, R. I.. Center For Development Of Nanoscience And Nanotechnology; Chile. Universidad Mayor; Chile
dc.description.institutionalaffiliationFil: Bringa, Eduardo Marcial. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza; Argentina. Universidad de Mendoza; Argentina. Universidad Mayor; Chile
dc.identifier.issn0927-0256
dc.identifier.urihttps://nuclea.cnea.gob.ar/handle/20.500.12553/8514
dc.publisherElsevier
dc.relationinfo:eu-repo/semantics/reference/hdl/11336/222596
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://linkinghub.elsevier.com/retrieve/pii/S0927025623002987
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1016/j.commatsci.2023.112304
dc.rights.licenseinfo:eu-repo/semantics/restrictedAccess
dc.rights.licensehttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subjectCORE–SHELL
dc.subjectIRRADIATION
dc.subjectMOLECULAR DYNAMICS
dc.subjectNANOPARTICLES
dc.subjectRADIATION-DAMAGE
dc.subjectOtras Ingeniería de los Materiales
dc.subjectIngeniería de los Materiales
dc.subjectINGENIERÍAS Y TECNOLOGÍAS
dc.subjectFísica Atómica, Molecular y Química
dc.subjectCiencias Físicas
dc.subjectCIENCIAS NATURALES Y EXACTAS
dc.subjectFísica de los Materiales Condensados
dc.subjectCiencias Físicas
dc.subjectCIENCIAS NATURALES Y EXACTAS
dc.titleProbing radiation resistance in simulated metallic core–shell nanoparticles
dc.typeARTÍCULO
dc.type.versionVersión publicada

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