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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1021/acs.jpcc.5b06211</dc:identifier><dc:language>eng</dc:language><dc:creator>Yangui, A.</dc:creator><dc:creator>Garrot, D.</dc:creator><dc:creator>Lauret, J. S.</dc:creator><dc:creator>Lusson, A.</dc:creator><dc:creator>Bouchez, G.</dc:creator><dc:creator>Deleporte, E.</dc:creator><dc:creator>Pillet, S.</dc:creator><dc:creator>Bendeif, E. E.</dc:creator><dc:creator>Castro, M.</dc:creator><dc:creator>Triki, S.</dc:creator><dc:creator>Abid, Y.</dc:creator><dc:creator>Boukheddaden, K.</dc:creator><dc:title>Optical investigation of broadband white-light emission in self-assembled organic-inorganic Perovskite (c6h11nh3)2pbbr4</dc:title><dc:identifier>ART-2015-92344</dc:identifier><dc:description>The performance of hybrid organic perovskite (HOP) for solar energy conversion is driving a renewed interest in their light emitting properties. The recent observation of broad visible emission in layered HOP highlights their potential as white-light emitters. Improvement of the efficiency of the material requires a better understanding of its photophysical properties. We present in-depth experimental investigations of white-light (WL) emission in thin films of the (C6H11NH3)2PbBr4. The broadband, strongly Stokes shifted emission presents a maximum at 90 K when excited at 3.815 eV, and below this temperature coexists with an excitonic edge emission. X-rays and calorimetry measurements exclude the existence of a phase transition as an origin of the thermal behavior of the WL luminescence. The free excitonic emission quenches at low temperature, despite a binding energy estimated to 280 meV. Time-resolved photoluminescence spectroscopy reveals the multicomponent nature of the broad emission. We analyzed the dependence of these components as a function of temperature and excitation energy. The results are consistent with the existence of self-trapped states. The quenching of the free exciton and the thermal evolution of the WL luminescence decay time are explained by the existence of an energy barrier against self-trapping, estimated to -10 meV.</dc:description><dc:date>2015</dc:date><dc:source>http://zaguan.unizar.es/record/65309</dc:source><dc:doi>10.1021/acs.jpcc.5b06211</dc:doi><dc:identifier>http://zaguan.unizar.es/record/65309</dc:identifier><dc:identifier>oai:zaguan.unizar.es:65309</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/MAT2013-44063-R</dc:relation><dc:identifier.citation>Journal of Physical Chemistry C 119, 41 (2015), 23638-23647</dc:identifier.citation><dc:rights>All rights reserved</dc:rights><dc:rights>http://www.europeana.eu/rights/rr-f/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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