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Recent Advances in Spiro-MeOTAD Hole Transport Material and Its Applications in Organic-Inorganic Halide Perovskite Solar Cells
Okinawa Institute of Science and Technology, JPN.ORCID iD: 0000-0001-9606-3521
Okinawa Institute of Science and Technology, JPN.ORCID iD: 0000-0003-3176-1876
Okinawa Institute of Science and Technology, JPN.ORCID iD: 0000-0002-4876-8049
2018 (English)In: Advanced Materials Interfaces, ISSN 2196-7350, Vol. 5, no 1, article id 1700623Article, review/survey (Refereed) Published
Abstract [en]

2,2,7,7-tetrakis-(N,N-di-4-methoxyphenylamino)-9,9-spirobifluorene (spiro-MeOTAD) hole transport material (HTM) is a milestone in the history of perovskite solar cells (PSCs). Proper choice of HTMs is key factor for efficient charge extraction and stability in solar cells. Spiro-MeOTAD is proven to be the most suitable HTM for testing PSCs due to its facile implementation and high performance. Similarly, spiro-MeOTAD is receiving attention in other applications other than in solar cells due to its desirable properties. However, spiro-MeOTAD is under debate regarding the topics of cost-performance, long-term stability, degradation issues (induced by temperature, additives, film quality, and environmental conditions), coating technologies compatibility, reliance on additives, and hysteresis. In this review, the advent of spiro-MeOTAD, and related aforementioned issues about spiro-MeOTAD are discussed. In addition, spiro-MeOTAD properties, alternative and new additives, other applications, and new HTMs that is comparable or outperforms spiro-MeOTAD in PSCs are summarized. In the outlook, the future research directions based on reported results that warrant further investigations are outlined.

Place, publisher, year, edition, pages
John Wiley & Sons, 2018. Vol. 5, no 1, article id 1700623
Keywords [en]
degradation, hole transport materials, perovskite solar cells, spiro-MeOTAD, stability
National Category
Materials Engineering
Research subject
Energy Technology
Identifiers
URN: urn:nbn:se:kau:diva-83185DOI: 10.1002/admi.201700623ISI: 000419675700004OAI: oai:DiVA.org:kau-83185DiVA, id: diva2:1530217
Available from: 2021-02-22 Created: 2021-02-22 Last updated: 2022-05-25Bibliographically approved

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Hawash, Zafer

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