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dc.contributor.authorRasmetyeva, A. V.en
dc.contributor.authorZyryanov, S. S.en
dc.contributor.authorNovoselov, I. E.en
dc.contributor.authorKukharenko, A. I.en
dc.contributor.authorMakarov, E. V.en
dc.contributor.authorCholakh, S. O.en
dc.contributor.authorKurmaev, E. Z.en
dc.contributor.authorZhidkov, I. S.en
dc.date.accessioned2025-02-25T10:52:06Z-
dc.date.available2025-02-25T10:52:06Z-
dc.date.issued2024-
dc.identifier.citationRasmetyeva, A., Zyryanov, S., Novoselov, I., Kukharenko, A., Makarov, E., Cholakh, S., Kurmaev, E., & Zhidkov, I. (2024). Proton Irradiation on Halide Perovskites: Numerical Calculations. Nanomaterials, 14(1), [1]. https://doi.org/10.3390/nano14010001apa_pure
dc.identifier.issn2079-4991-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access; Gold Open Access3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85181931776&doi=10.3390%2fnano14010001&partnerID=40&md5=bbafef178d58472fc35aba5096dd7d571
dc.identifier.otherhttps://www.mdpi.com/2079-4991/14/1/1/pdf?version=1702956244pdf
dc.identifier.urihttp://elar.urfu.ru/handle/10995/141652-
dc.description.abstractThe results of numerical SRIM and SCAPS calculations for the ionization, displacement and heating of hybrid perovskites under the influence of protons (E = 0.15, 3.0 and 18 MeV) are presented and show that the lowest transfer energy is demonstrated by the MAPbI3, FAPbBr3 and FAPbI3 compounds, which represent the greatest potential for use as solar cells in space devices. On the other hand, it is found that perovskite compositions containing FA and Cs and with mixed cations are the most stable from the point of view of the formation of vacancies and phonons and are also promising as radiation-resistant materials with respect to powerful proton fluxes. Taking into account the lateral distribution of proton tracks showed that, at an energy level of several MeV, the release of their energy can be considered uniform over the depth and area of the entire solar cell, suggesting that the simple protection by plastic films from the low-energy protons is sufficient. © 2023 by the authors.en
dc.description.sponsorshipMinistry of Education and Science of the Russian Federation, Minobrnauka, (AAAA-A18-118020190098-5); Ministry of Education and Science of the Russian Federation, Minobrnauka; Russian Science Foundation, RSF, (22-61-00047); Russian Science Foundation, RSFen
dc.description.sponsorshipThis work was supported by the Russian Science Foundation (Project 22-61-00047). E.Z.K. thanks support by the Ministry of Science and Higher Education of the Russian Federation under the theme “Electron” No. AAAA-A18-118020190098-5.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherMultidisciplinary Digital Publishing Institute (MDPI)en
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.rightscc-byother
dc.sourceNanomaterials2
dc.sourceNanomaterialsen
dc.subjectHYBRID PEROVSKITESen
dc.subjectPROTON IRRADIATIONen
dc.subjectSCAPSen
dc.subjectSRIMen
dc.subjectSTABILITYen
dc.titleProton Irradiation on Halide Perovskites: Numerical Calculationsen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.3390/nano14010001-
dc.identifier.scopus85181931776-
local.contributor.employeeRasmetyeva A.V., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federationen
local.contributor.employeeZyryanov S.S., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federationen
local.contributor.employeeNovoselov I.E., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federationen
local.contributor.employeeKukharenko A.I., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federation, M.N. Mikheev Institute of Metal Physics of Ural Branch of Russian Academy of Sciences, S. Kovalevskoi 18 Street, Yekaterinburg, 620108, Russian Federationen
local.contributor.employeeMakarov E.V., Institute of Electrophysics of Ural Branch of Russian Academy of Sciences, Amundsena 106 Street, Yekaterinburg, 620110, Russian Federationen
local.contributor.employeeCholakh S.O., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federationen
local.contributor.employeeKurmaev E.Z., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federation, M.N. Mikheev Institute of Metal Physics of Ural Branch of Russian Academy of Sciences, S. Kovalevskoi 18 Street, Yekaterinburg, 620108, Russian Federationen
local.contributor.employeeZhidkov I.S., Institute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federation, M.N. Mikheev Institute of Metal Physics of Ural Branch of Russian Academy of Sciences, S. Kovalevskoi 18 Street, Yekaterinburg, 620108, Russian Federationen
local.issue1-
local.volume14-
dc.identifier.wos001140375800001-
local.contributor.departmentInstitute of Physics and Technology, Ural Federal University, Mira 19 Street, Yekaterinburg, 620002, Russian Federationen
local.contributor.departmentM.N. Mikheev Institute of Metal Physics of Ural Branch of Russian Academy of Sciences, S. Kovalevskoi 18 Street, Yekaterinburg, 620108, Russian Federationen
local.contributor.departmentInstitute of Electrophysics of Ural Branch of Russian Academy of Sciences, Amundsena 106 Street, Yekaterinburg, 620110, Russian Federationen
local.identifier.pure51597086-
local.description.order1
local.identifier.eid2-s2.0-85181931776-
local.fund.rsfMinistry of Education and Science of the Russian Federation, Minobrnauka, (AAAA-A18-118020190098-5); Ministry of Education and Science of the Russian Federation, Minobrnauka; 22-61-00047
local.identifier.wosWOS:001140375800001-
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