Operando Raman and UV-Vis spectroscopic investigation of the coloring and bleaching mechanism of self-powered photochromic devices for smart windows

Nano Energy ◽  
2021 ◽  
Vol 82 ◽  
pp. 105721
Author(s):  
So Yeon Chun ◽  
Sunghyeok Park ◽  
Seok In Lee ◽  
Hieu Dinh Nguyen ◽  
Kyung-Koo Lee ◽  
...  
1995 ◽  
Vol 377 ◽  
Author(s):  
John N. Bullock ◽  
Yueqin Xu ◽  
David Benson ◽  
Howard M. Branz

ABSTRACTSelf-powered “smart” windows utilize an electro-optic transmittance modulator based on electrochromic (EC) thin films that exhibit reversible and controlled changes in optical properties with an applied voltage between 0.7 and 2.0 V. Existing window designs require an external electrical connection, which may be economically unfeasible. This problem is solved by the tandem photovoltaic-electrochromic device, in which a wide-gap amorphous silicon-based alloy photovoltaic device is deposited together with an electrochromic optical transmittance modulator in a monolithic device on a single substrate. In this paper, we discuss our proposed monolithic photovoltaic-electrochromic device.We also present studies of transparent, wide-gap (1.8 to 2.2 eV) amorphous silicon-carbon thin films and p-i-n devices designed for use in the photovoltaic-electrochromic device. These photovoltaic cells can operate at low current (<1 mA/cm2) because a total injected charge of only 60 μC/cm2 will darken the EC layer to a visible transmission of 5%, but they need a high open-circuit voltage (>1.0 V) and high transparency (≈70%). We present our progress toward these design targetxxss.


2019 ◽  
Vol 55 (80) ◽  
pp. 12060-12063 ◽  
Author(s):  
Jinzi Sun ◽  
Ying Li ◽  
Jiankun Sun ◽  
Zhijun Zhu ◽  
Yanling Zhai ◽  
...  

Self-powered electrofluorochromic devices (EFCDs) have attracted particular attention for smart windows of green buildings.


Nano Energy ◽  
2021 ◽  
Vol 90 ◽  
pp. 106575
Author(s):  
Chao-Yuan Cheng ◽  
Yu-Jou Chiang ◽  
Hsin-Fu Yu ◽  
Li-Yin Hsiao ◽  
Chia-Lin Yeh ◽  
...  

1965 ◽  
Vol 5 ◽  
pp. 120-130
Author(s):  
T. S. Galkina

It is necessary to have quantitative estimates of the intensity of lines (both absorption and emission) to obtain the physical parameters of the atmosphere of components.Some years ago at the Crimean observatory we began the spectroscopic investigation of close binary systems of the early spectral type with components WR, Of, O, B to try and obtain more quantitative information from the study of the spectra of the components.


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