scholarly journals Transient absorption spectroscopy of polymer-based thin-film solar cells

Polymer ◽  
2011 ◽  
Vol 52 (20) ◽  
pp. 4397-4417 ◽  
Author(s):  
Hideo Ohkita ◽  
Shinzaburo Ito
2016 ◽  
Vol 18 (13) ◽  
pp. 8938-8944 ◽  
Author(s):  
Iulia Minda ◽  
Essraa Ahmed ◽  
Vivien Sleziona ◽  
Christoph Richter ◽  
Max Beu ◽  
...  

Charge transfer dynamics in fully operational dye sensitised solar cells as observed using ultrafast transient absorption spectroscopy.


2015 ◽  
Vol 17 (22) ◽  
pp. 14674-14684 ◽  
Author(s):  
Piotr Piatkowski ◽  
Boiko Cohen ◽  
Francisco Javier Ramos ◽  
Maria Di Nunzio ◽  
Mohammad Khaja Nazeeruddin ◽  
...  

Electron and hole dynamics, and internal and surface trap states in perovskite-based solar cells are explored by fs transient absorption spectroscopy.


2021 ◽  
Vol 11 (8) ◽  
pp. 2003446
Author(s):  
Yu‐Han Chang ◽  
Romain Carron ◽  
Mario Ochoa ◽  
Carlota Bozal‐Ginesta ◽  
Ayodhya N. Tiwari ◽  
...  

2016 ◽  
Vol 2016 ◽  
pp. 1-17 ◽  
Author(s):  
Yutaka Moritomo ◽  
Kouhei Yonezawa ◽  
Takeshi Yasuda

Subpicosecond transient absorption spectroscopy is a powerful tool used to clarify the exciton and carrier dynamics within the organic solar cells (OSCs). In this review article, we introduce a method to determine the absolute numbers of the excitons and carriers against delay time (t) only from the photoinduced absorption (PIA) and electrochemically induced absorption (EIA) spectra. Application of this method to rr-P3HT-, PTB7-, and SMDPPEH-based OSCs revealed common aspects of the carrier formation dynamics. First, the temporal evolution of the numbers of the excitons and carriers indicates that the late decay component of exciton does not contribute to the carrier formation process. This is probably because the late component has not enough excess energy to separate into the electron and hole across the donor/acceptor (D/A) interface. Secondly, the spectroscopy revealed that the exciton-to-carrier conversion process is insensitive to temperature. This observation, together with the fast carrier formation time in OSCs, is consistent with the hot exciton picture.


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