{"id":1726,"date":"2019-03-25T10:43:08","date_gmt":"2019-03-25T10:43:08","guid":{"rendered":"http:\/\/grupodeespectroscopia.es\/MW\/?p=1726"},"modified":"2019-03-27T16:18:23","modified_gmt":"2019-03-27T16:18:23","slug":"our-research-about-degradation-mechanism-and-relative-stability-of-methylammonium-halide-based-perovskites-accepted-in-acs-applied-materials-and-interfaces-journal","status":"publish","type":"post","link":"https:\/\/grupodeespectroscopia.es\/MW\/our-research-about-degradation-mechanism-and-relative-stability-of-methylammonium-halide-based-perovskites-accepted-in-acs-applied-materials-and-interfaces-journal\/","title":{"rendered":"Our research about Degradation Mechanism and Relative Stability of Methylammonium Halide Based Perovskites accepted in ACS Applied Materials and Interfaces Journal"},"content":{"rendered":"<p style=\"text-align: left;\">The correct identification of all gases released during hybrid perovskite degradation is of great significance to develop strategies to extend the lifespan of any device based on this semiconductor. CH<sub>3<\/sub>X (X = Br\/I) is a released degradation gas\/low boiling point liquid arising from methylammonium (MA<sup>+<\/sup>) based perovskites, which has been largely overlooked in the literature focusing on stability of perovskite solar cells. Herein, we present an unambiguous identification of CH<sub>3<\/sub>I release using microwave (rotational) spectroscopy. An experimental back-reaction test demonstrates that the well-known CH<sub>3<\/sub>NH<sub>2<\/sub>\/HX degradation route may not be the ultimate degradation pathway of MAPbX<sub>3<\/sub> in thermodynamic closed systems. Meanwhile, the CH<sub>3<\/sub>X\/NH<sub>3<\/sub> route cannot back-react selectively to MAX formation as occurred for the former back-reaction. Metadynamics calculations uncover the X halide effect on energy barriers for both degradation reactions showing a better stability of Br based perovskite ascribed to two aspects: (i) lower Br\u00f6nsted\u2212Lowry acidity of HBr compared to HI and (ii) higher nucleophilic character of CH<sub>3<\/sub>NH<sub>2<\/sub> compared to NH<sub>3<\/sub>. The latter property makes CH<sub>3<\/sub>NH<sub>2<\/sub> molecules stay preferentially attached on the electrophilic perovskite surface (Pb<sup>2+<\/sup>) during the dynamic simulation instead of being detached as observed for the NH<sub>3<\/sub> molecule.<\/p>\n<p><img decoding=\"async\" loading=\"lazy\" class=\"aligncenter size-full wp-image-1727\" src=\"http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2019\/03\/Captura-de-pantalla-2019-03-25-a-las-9.04.04.png\" alt=\"\" width=\"415\" height=\"212\" srcset=\"https:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2019\/03\/Captura-de-pantalla-2019-03-25-a-las-9.04.04.png 415w, https:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2019\/03\/Captura-de-pantalla-2019-03-25-a-las-9.04.04-300x153.png 300w\" sizes=\"(max-width: 415px) 100vw, 415px\" \/><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The correct identification of all gases released during hybrid perovskite degradation is of great significance to develop strategies to extend the lifespan of any device based on this semiconductor. CH3X (X = Br\/I) is a released degradation gas\/low boiling point liquid arising from methylammonium (MA+) based perovskites, which has been largely overlooked in the literature &hellip;<\/p>\n","protected":false},"author":1,"featured_media":1727,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":[],"categories":[1,29],"tags":[],"acf":[],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/posts\/1726"}],"collection":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/comments?post=1726"}],"version-history":[{"count":3,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/posts\/1726\/revisions"}],"predecessor-version":[{"id":1736,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/posts\/1726\/revisions\/1736"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/media\/1727"}],"wp:attachment":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/media?parent=1726"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/categories?post=1726"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/tags?post=1726"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}