Yang Zhang (30734)Ruizhi Wang (508892)Yezhou Li (1428364)Zeyang Wang (3873793)Shu Hu (267877)Xiaoliang Yan (1945372)Yaxin Zhai (2562517)Chuang Zhang (2199421)ChuanXiang Sheng (6101819)
The\ntemperature dependence of absorption and photoluminescence\n(PL) spectroscopies were used to study the optical properties of 2D\nperovskite films, including <i>n</i> = 1 and 3 of (PEA)<sub>2</sub>(CH<sub>3</sub>NH<sub>3</sub>)<sub><i>n</i>−1</sub>[Pb<sub><i>n</i></sub>I<sub>3<i>n</i>+1</sub>] (PEA = C<sub>6</sub>H<sub>5</sub>(CH<sub>2</sub>)<sub>2</sub>NH<sub>3</sub>). In (PEA)<sub>2</sub>[Pb<sub>1</sub>I<sub>4</sub>] (PEPI),\nexcitons coupling to optical phonons with an average energy of ∼30\nmeV dominate the photophysics of absorption and PL. (PEA)<sub>2</sub>(CH<sub>3</sub>NH<sub>3</sub>)<sub>2</sub>[Pb<sub>3</sub>I<sub>10</sub>] (shortened as PMPI<sub>3</sub>), nominally prepared as <i>n</i> = 3, actually was a mixture of multiple layered perovskites\nwith various <i>n</i>. In absorption, a PMPI<sub>3</sub> film presents respective <i>n</i> materials’ excitonic\nfeatures, coupling to phonons with an average energy of ∼30\nmeV; in analyzing PL peaked singly at ∼1.6 eV and its width\nas a function of temperature, we found that PMPI<sub>3</sub> behaves\nlike PEPI at around 80 K but like 3D perovskite near room temperature,\nwith three times larger electron–phonon interaction strength\ncompared to that in PEPI.
Yunling Liu (1420054)Zhan Shi (704217)Yunlong Fu (1536427)Wei Chen (23863)Baozong Li (1621120)Jia Hua (410225)Wuyang Liu (2953659)Feng Deng (553812)Wenqin Pang (2537944)
Junghwan Do (2102317)Ranko P. Bontchev (2425492)Allan J. Jacobson (1644922)
Evan L. Werkema (1782670)Ludovic Castro (1472713)Laurent Maron (1346082)Odile Eisenstein (1358145)Richard A. Andersen (244546)
Stanislav I. Stoliarov (3051027)Vadim D. Knyazev (1464019)Irene R. Slagle (2731753)
Stanislav I. Stoliarov (3051027)Vadim D. Knyazev (1464019)Irene R. Slagle (2731753)