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Date

2021-06-17

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Creative Commons
Except where otherwise noted, this item's license is described as Attribution 4.0 International

Recently, ternary copper(I) halides have emerged as alternatives to lead halide perovskites for light emission applications. Despite their high-efficiency photoluminescence (PL) properties, most copper(I) halides are blue emitters with unusually poor tunability of their PL properties. Here, we report the impact of substitution of copper with silver in the high-efficiency blue-emitting Cu(I) halides through hydrothermal synthesis and characterization of (NH4)2AgX3 (X = Br, I). (NH4)2AgX3 are found to exhibit contrasting light emission properties compared to the blue-emitting Cu(I) analogues. Thus, (NH4)2AgBr3 and (NH4)2AgI3 exhibit broadband whitish light emission at room temperature with PL maxima at 394 and 534 nm and full width at half-maximum values of 142 and 114 nm, respectively. Based on our combined experimental and computational results, the broadband emission in (NH4)2AgX3 is attributed to the presence of high-stability self-trapped excitons and defect-bound excitons. (NH4)2AgBr3 and (NH4)2AgI3 both have significantly improved air and moisture stability as compared to the related copper(I) halides, which are prone to degradation via oxidation. Our results suggest that silver halides should be considered alongside their copper analogues for high-efficiency light emission applications.

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Keywords

Inorganic compounds, Crystal structure, Light, Silver, Halogens, Photoluminescence, Lead−free halides, Silver halides, Light emission, STE

Citation

ACS Mater. Au 2021, XXXX, XXX, XXX-XXX. https://doi.org/10.1021/acsmaterialsau.1c00011

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Sponsorship

This material is based upon work supported by the National Aeronautics and Space Administration under Agreement No.80NSSC19M0140 issued through NASA Oklahoma EPSCoR.M.-H.D. was supported by the U.S. Department of Energy,Office of Science, Basic Energy Sciences, Materials Sciences,and Engineering Division. Open Access fees paid for in whole or in part by the University of Oklahoma Libraries.