Reverse dark current in organic photodetectors and the major role of traps as source of noise

Kublitski, Jonas;Hofacker, Andreas;K. Boroujeni, Bahman;Benduhn, Johannes;C. Nikolis, Vasileios;Kaiser, Christina;Spoltore, Donato;Kleemann, Hans;Fischer, Axel;Ellinger, Frank;Vandewal, Koen;Leo, Karl

Description

Organic photodetectors have promising applications in low-cost imaging, health monitoring and near infrared sensing. Recent research on organic photodetectors based on donor-acceptor systems has resulted in narrow-band, flexible and biocompatible devices, of which the best reach external photovoltaic quantum efficiencies approaching 100%. However, the high noise spectral density of these devices limits their specific detectivity to around 10^13 Jones in the visible and several orders of magnitude lower in the near-infrared, severely reducing performance. Here, we show that the shot noise, proportional to the dark current, dominates the noise spectral density, demanding a comprehensive understanding of the dark current. We demonstrate that, in addition to the intrinsic saturation current generated via charge-transfer states, dark current contains a major contribution from trap-assisted generated charges and decreases systematically with decreasing concentration of traps. By modeling the dark current of several donor-acceptor systems, we reveal the interplay between traps and charge-transfer states as source of dark current and show that traps dominate the generation processes, thus being the main limiting factor of organic photodetectors detectivity.

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Metrics

Dataset Index

1.4

FAIR Score

77%

Citations

1

Mentions

0

Metrics Over Time

Publication Details

DOI

Publisher

Materials Cloud

License

Creative Commons Attribution 4.0 International

Assigned Domain

Subfield

Instrumentation

Field

Physics and Astronomy

Domain

Physical Sciences

Confidence Score

51%

Source

Scholar Data Model

Keywords

Organic PhotodetectorsDark currentTrapsDetectivity

Normalization Factors

FT

26.92

CTw

1.00

MTw

1.00