Design, synthesis and theoretical simulations of novel spiroindane-based enamines as p -type semiconductors

Author:

Daskeviciute-Geguziene Sarune1,Daskeviciene Maryte1,Kantminienė Kristina2ORCID,Jankauskas Vygintas3,Kamarauskas Egidijus3,Gruodis Alytis3,Karazhanov Smagul4,Getautis Vytautas1

Affiliation:

1. Department of Organic Chemistry, Kaunas University of Technology, Kaunas 50254, Lithuania

2. Department of Physical and Inorganic Chemistry, Kaunas University of Technology, Kaunas, 50254, Lithuania

3. Institute of Chemical Physics, Vilnius University, Vilnius, 10257, Lithuania

4. Institute for Energy Technology (IFE), Kjeller 2027, Norway

Abstract

The search for novel classes of hole-transporting materials (HTMs) is a very important task in advancing the commercialization of various photovoltaic devices. Meeting specific requirements, such as charge-carrier mobility, appropriate energy levels and thermal stability, is essential for determining the suitability of an HTM for a given application. In this work, two spirobisindane-based compounds, bearing terminating hole transporting enamine units, were strategically designed and synthesized using commercially available starting materials. The target compounds exhibit adequate thermal stability; they are amorphous and their glass-transition temperatures (>150°C) are high, which minimizes the probability of direct layer crystallization. V1476 stands out with the highest zero-field hole-drift mobility, approaching 1 × 10 −5 cm 2 V s −1 . To assess the compatibility of the highest occupied molecular orbital energy levels of the spirobisindane-based HTMs in solar cells, the solid-state ionization potential ( I p ) was measured by the electron photoemission in air of the thin-film method. The favourable morphological properties, energy levels and hole mobility in combination with a simple synthesis make V1476 and related compounds promising materials for HTM applications in antimony-based solar cells and triple-cation-based perovskite solar cells.

Publisher

The Royal Society

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