dc.creator | Yaccuzzi, Exequiel Eliseo | |
dc.creator | Di Napoli, Solange Mariel | |
dc.creator | Di Liscia, Emiliano Javier | |
dc.creator | Suárez, Sergio Ariel | |
dc.creator | Alurralde, Martín Alejo | |
dc.creator | Strittmatter, Andre | |
dc.creator | Pla, Juan Carlos | |
dc.creator | Giudici, Paula | |
dc.date.accessioned | 2021-11-11T04:27:52Z | |
dc.date.accessioned | 2022-10-15T05:03:57Z | |
dc.date.available | 2021-11-11T04:27:52Z | |
dc.date.available | 2022-10-15T05:03:57Z | |
dc.date.created | 2021-11-11T04:27:52Z | |
dc.date.issued | 2020-01 | |
dc.identifier | Yaccuzzi, Exequiel Eliseo; Di Napoli, Solange Mariel; Di Liscia, Emiliano Javier; Suárez, Sergio Ariel; Alurralde, Martín Alejo; et al.; Experimental re-evaluation of proton penetration ranges in GaAs and InGaP; IOP Publishing; Journal of Physics D: Applied Physics; 54; 11; 1-2020; 115302 | |
dc.identifier | 0022-3727 | |
dc.identifier | http://hdl.handle.net/11336/146635 | |
dc.identifier | CONICET Digital | |
dc.identifier | CONICET | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4347828 | |
dc.description.abstract | Multijunction solar cells based on InGaP and GaAs materials are currently the state of the art for space applications due to their high eciencies. However, the space is a hazardous environment with di↵erent energetic particles that degrade the solar cell eciency, hence decreasing the satellite lifetime. To gain insight in the behaviour of the solar cells under particle bombardment, we study the e↵ect of radiation on InGaP and GaAs layers, constituent materials of III-V solar cells. By means of Photoluminescence and Raman spectroscopy we investigate changes of the optical parameters in the irradiated region, and compare the results with simulations obtained with the code Stopping and Ranges of Ions in Matter. The proton ranges obtained from experiments di↵er considerably from the predicted by the simulations in the case of InGaP. We demonstrate that this discrepancy increases monotonously with proton energy. We discuss the possible origin of the di↵erences in terms of electronic orbitals and bonding structure of the simulated compound, and the implications in the design of solar cells for space applications. | |
dc.language | eng | |
dc.publisher | IOP Publishing | |
dc.relation | info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1361-6463/abce7d | |
dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/1361-6463/abce7d | |
dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | |
dc.rights | info:eu-repo/semantics/restrictedAccess | |
dc.subject | III-V COMPOUNDS | |
dc.subject | MULTIJUNCTION SOLAR CELLS | |
dc.subject | RADIATION DAMAGE | |
dc.subject | RAMAN SPECTROSCOPY | |
dc.subject | SPACE APPLICATIONS | |
dc.title | Experimental re-evaluation of proton penetration ranges in GaAs and InGaP | |
dc.type | info:eu-repo/semantics/article | |
dc.type | info:ar-repo/semantics/artículo | |
dc.type | info:eu-repo/semantics/publishedVersion | |