Molybdenum nitride (MoN) was perceived as carrier-selective contacts (CSCs) for crystalline silicon (c-Si) solar cells due to having proper work functions and excellent conductivities. However, the poor passivation and non-Ohmic contact at the c-Si/MoN interface endow an inferior hole selectivity. Here, the surface, interface, and bulk structures of MoN films are systematically investigated by X-ray scattering, surface spectroscopy, and electron microscope analysis to reveal the carrier-selective features. Surface layers with the composition of MoON form upon air exposure, which induces the overestimated work function and explains the origin of inferior hole selectivities. The c-Si/MoN interface is confirmed to adopt long-term stability, providing guidance for designing stable CSCs. A detailed evolution of the scattering length density, domain sizes, and crystallinity in the bulk phase is presented to elucidate its superior conductivity. These multiscale structural investigations offer a clear structure-function correlation of MoN films, providing key inspiration for developing excellent CSCs for c-Si solar cells.

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http://dx.doi.org/10.1021/acsami.2c22781DOI Listing

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