Pesci Martina, Romagnoli Lorenza, Brunetti Bruno, Vecchio Ciprioti Stefano, Ciccioli Andrea, Latini Alessandro
Dipartimento di Chimica, Sapienza University of Rome, P.le A. Moro 5, Rome 00185, Italy.
Istituto per lo Studio dei Materiali Nanostrutturati, Consiglio Nazionale delle Ricerche, Dipartimento di Chimica, Sapienza University of Rome, P.le A. Moro 5, Rome 00185, Italy.
J Phys Chem C Nanomater Interfaces. 2025 May 10;129(20):9291-9301. doi: 10.1021/acs.jpcc.5c01854. eCollection 2025 May 22.
The gas-releasing thermal decomposition processes of formamidinium tin triiodide perovskite (CNHSnI, usually denoted as FASnI or, briefly, FASI) were investigated in order to obtain information on the temperature at which decomposition begins and on the nature of the gas species emitted under heating. Results of thermogravimetry-differential thermal analysis (TG-DTA), thermogravimetry-differential scanning calorimetry (TG-DSC), and Knudsen effusion mass spectrometry (KEMS) experiments are presented. TG measurements showed that mass loss starts at temperatures much lower than those of the lead-based corresponding compound FAPbI, with incipient loss at temperatures as low as 423 K. Unlike FAPbI, practically no residue is left at = 823 K. KEMS experiments showed a measurable release of SnI(g) occurring from temperatures as low as 318 K, with a SnI(g) pressure much lower than the vapor pressure of pure SnI, suggesting the presence in the solid of Sn-(IV) at reduced activity. At higher temperatures ( > 390 K), the release of SnI(g) and various species coming from the organic portion, such as formamidine, hydrogen iodide, ammonia, triazine, and hydrogen cyanide, is observed. For the first time, thermal decomposition of FASI was shown to occur with release of both organic and inorganic (tin iodides) species, with the partial oxidation of Sn-(II) to Sn-(IV) significantly decreasing the decomposition onset temperature. Finally, based on TG measurements at various scan rates, a kinetic analysis of FASI decomposition was performed, using integral and incremental isoconversional methods, to derive parameters useful for lifetime prediction. Reasonable reaction time values to achieve a low degree of conversion (less than 0.25) were extrapolated at temperatures typically involved in the operation of photovoltaic devices (333 to 353 K).
为了获取关于甲脒三碘化锡钙钛矿(CNHSnI,通常表示为FASnI或简称为FASI)热分解开始的温度以及加热时释放的气体种类的性质的信息,对其气体释放热分解过程进行了研究。本文展示了热重-差热分析(TG-DTA)、热重-差示扫描量热法(TG-DSC)和克努森 effusion 质谱(KEMS)实验的结果。TG测量表明,质量损失在远低于相应的铅基化合物FAPbI的温度下开始,在低至423K的温度下开始有初始损失。与FAPbI不同,在823K时几乎没有残留物。KEMS实验表明,从低至318K的温度开始就有可测量的SnI(g)释放,SnI(g)的压力远低于纯SnI的蒸气压,这表明固体中存在活性降低的Sn-(IV)。在较高温度(>390K)下,观察到SnI(g)以及来自有机部分的各种物质的释放,如甲脒、碘化氢氨、三嗪和氰化氢。首次表明FASI的热分解伴随着有机和无机(碘化锡)物质的释放,Sn-(II)部分氧化为Sn-(IV)显著降低了分解起始温度。最后,基于不同扫描速率下的TG测量,使用积分和增量等转化率方法对FASI分解进行了动力学分析,以得出有助于寿命预测的参数。在光伏器件运行通常涉及的温度(333至353K)下,外推了达到低转化率(小于0.25)的合理反应时间值。