2021
DOI: 10.1021/acsenergylett.1c00458
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Charge-Carrier Mobility and Localization in Semiconducting Cu2AgBiI6 for Photovoltaic Applications

Abstract: Lead-free silver–bismuth semiconductors have become increasingly popular materials for optoelectronic applications, building upon the success of lead halide perovskites. In these materials, charge-lattice couplings fundamentally determine charge transport, critically affecting device performance. In this study, we investigate the optoelectronic properties of the recently discovered lead-free semiconductor Cu2AgBiI6 using temperature-dependent photoluminescence, absorption, and optical-pump terahertz-probe spec… Show more

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Cited by 47 publications
(98 citation statements)
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“…We also note the presence of some subgap absorption between approximately 950−700 nm, as measured by Fourier transform infrared (FTIR) spectroscopy, which is possibly due to subgap defect states similar to those observed by Photo-Thermal Deflection Spectroscopy (PDS) in Cu 2 AgBiI 6 , although we cannot rule out scattering of longwavelength light from the rough film surfaces leading to lower light transmission in this region but still allowing for the red transmitted light observed when the films are backlit (Figure S7f). We measure steady-state photoluminescence (PL) spectra on the same thin film under continuous wave excitation in vacuum, with CuAgBiI 5 showing weak, broad emission peaking at approximately 760 nm (1.63 eV), giving a Stokes shift of 390 meV, similar to, though slightly larger than, that observed in Cu 2 AgBiI 6 and characteristic of emission from localized charge-carrier states, which has been proposed as the source of PL emission in Cu 2 AgBiI 6 , 25 as well as for Cs 2 AgBiBr 6 (Figure 7a). 6,38,39 Compared to Cu 2 AgBiI 6 , the PL peak of CuAgBiI 5 is slightly shifted to lower energies (1.71 eV for Cu 2 AgBiI 6 ) with a slightly higher Stokes shift (350 meV for Cu 2 AgBiI 6 ).…”
Section: ■ Common Structural Featuresmentioning
confidence: 71%
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“…We also note the presence of some subgap absorption between approximately 950−700 nm, as measured by Fourier transform infrared (FTIR) spectroscopy, which is possibly due to subgap defect states similar to those observed by Photo-Thermal Deflection Spectroscopy (PDS) in Cu 2 AgBiI 6 , although we cannot rule out scattering of longwavelength light from the rough film surfaces leading to lower light transmission in this region but still allowing for the red transmitted light observed when the films are backlit (Figure S7f). We measure steady-state photoluminescence (PL) spectra on the same thin film under continuous wave excitation in vacuum, with CuAgBiI 5 showing weak, broad emission peaking at approximately 760 nm (1.63 eV), giving a Stokes shift of 390 meV, similar to, though slightly larger than, that observed in Cu 2 AgBiI 6 and characteristic of emission from localized charge-carrier states, which has been proposed as the source of PL emission in Cu 2 AgBiI 6 , 25 as well as for Cs 2 AgBiBr 6 (Figure 7a). 6,38,39 Compared to Cu 2 AgBiI 6 , the PL peak of CuAgBiI 5 is slightly shifted to lower energies (1.71 eV for Cu 2 AgBiI 6 ) with a slightly higher Stokes shift (350 meV for Cu 2 AgBiI 6 ).…”
Section: ■ Common Structural Featuresmentioning
confidence: 71%
“…We measure steady-state photoluminescence (PL) spectra on the same thin film under continuous wave excitation in vacuum, with CuAgBiI 5 showing weak, broad emission peaking at approximately 760 nm (1.63 eV), giving a Stokes shift of 390 meV, similar to, though slightly larger than, that observed in Cu 2 AgBiI 6 and characteristic of emission from localized charge-carrier states, which has been proposed as the source of PL emission in Cu 2 AgBiI 6 , as well as for Cs 2 AgBiBr 6 (Figure a). ,, Compared to Cu 2 AgBiI 6 , the PL peak of CuAgBiI 5 is slightly shifted to lower energies (1.71 eV for Cu 2 AgBiI 6 ) with a slightly higher Stokes shift (350 meV for Cu 2 AgBiI 6 ). The PL peak of the CuAgBiI 5 thin film is fitted to a Gaussian peak shape with an fwhm of 312(6) meV, slightly wider than the fwhm of 289 meV extracted for Cu 2 AgBiI 6 films.…”
Section: Properties Of 3d Cuagbii5 Compared To 2d Cu2agbii6mentioning
confidence: 90%
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“…The extracted mobility and its temperature dependence are presented in Figure 3 I, which illustrates an increase of μ with decreasing temperature. In general, the temperature dependence of charge-carrier mobility is closely related to the charge scattering mechanism in the semiconductors and can be expressed as ( Biewald et al., 2019 ; Wright et al., 2016 ), where γ reflects the magnitude of charge scattering, with larger γ representing stronger scattering in the perovskite ( Buizza et al., 2021 ; Herz, 2017 ; Senanayak et al., 2017 ). The pristine device shows a γ value of 1.47 between 200 and 280 K, which seems to indicate the charge transport in this regime is dominated by acoustic phonon scattering ( Biewald et al., 2019 ; Wright et al., 2016 ; Yi et al., 2016 ).…”
Section: Resultsmentioning
confidence: 99%
“…In contrast, no change or minor red-shifts in photoluminescence have been observed for Cs 2 AgBiBr 6 , accompanied by a slight narrowing of the emission line width (∼20 meV). 39 For some of the halide double perovskites (e.g., Cu 2 AgBiI 6 , 40 Rb 4 Ag 2 BiBr 9 41 ), even more complex low-temperature spectra have been observed, showing multiple peaks also in the near-infrared region of the spectrum. The origin of the emission feature is still heavily under debate.…”
mentioning
confidence: 99%