PbI perovskite solar cells consisted of RF sputtered NiOx as hole transport layer
Masatoshi Yanagida a c, Md Bodiul Islam b, Namrata Pant c, Yasuhiro Shirai a, Kenjiro Miyano a
a Global Research Center for Environment and Energy based on Nanomaterials Science (GREEN), National Institute for Materials Science (NIMS)
b Department of Glass and Ceramic Engineering, Rajshahi University of Engineering & Technology
c Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi
International Conference on Hybrid and Organic Photovoltaics
Proceedings of International Conference on Hybrid and Organic Photovoltaics (HOPV18)
Benidorm, Spain, 2018 May 28th - 31st
Organizers: Emilio Palomares and Rene Janssen
Poster, Masatoshi Yanagida, 218
Publication date: 21st February 2018

 

PbI perovskite (PVK) solar cells have been intensively investigated because the PVK has the large absorption coefficient (> 104 cm-1) in the visible region and long carrier diffusion length (>1 mm). We have investigated planar type PVK solar cells consisted of ITO / NiOx / PVK / PCBM /Ag to produce the solar cells via lower temperature production processes. We have prepared radio-frequency (RF) sputtered NiOx films as hole transport layer because of the high stability under continuous illumination of solar light (1-2). We sputtered NiOx films by using NiO as the sputtering target. The property of NiOx films depends on the sputtering conditions such as Ar gas pressure, and the sputtering power. The sheet resistance of NiOx films decreases with decrease of Ar pressure. The transmittance also decreases in the visible and near-IR region. From XPS, the large amount of Ni3+ increases with decrease of Ar pressure. The short circuit current density of PVK solar cells decreases with decrease of Ar pressure because of low transmittance. The shunt resistance and VOC do not decrease. Therefore, the Ni3+ does not act as recombination center. 

 

(1) M. Yanagida, L. Shimomoto, Y. Shirai, and K. Miyano, Electrochemistry, 85, 231 (2017).

 

(2) Md. B. Islam, M. Yanagida, Y. Shirai, Y. Nabetani, and K. Miyano, ACS Omega 2, 2291 (2017).

 

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