Researchers at the University of Rome Tor Vergata in Italy and Russia's NUST MISIS institute have investigated how cells containing two-dimensional titanium-carbide MXene support layers could improve perovskite solar cell performance.
To obtain good power conversion within a perovskite solar cell, all layers and layer interfaces within the cell must have good compatibility. Typical cells contain the active perovskite material sandwiched between two charge transport layers, which are then adjacent to their corresponding electrodes. Support layers may also be added. Charge mobility, energy barriers, interface energy alignment, and interfacial vacancies all impact compatibility and subsequent cell performance and stability. Thus, engineering well-suited interfaces with the cell is paramount to cell success and long-term stability, an important criterion for potential commercialization.
The team utilized titanium-carbide MXenes, Ti3C2Tx, where T can be oxygen, hydroxide, or fluoride, as buffer layers within perovskite solar cells. By inserting these MXenes in between active material layers in their functional perovskite solar cell, they demonstrated an impressive cell efficiency of 20.14%. The fill factor, a quantification of the maximum power generated by a solar cell, was 77.6%. The short circuit current density, or largest current to be drawn from the cell, was 23.82 mA/cm2. The maximum possible voltage, called the open circuit voltage, was 1.09 V. For comparison, commercially available silicon solar cells have a typical cell efficiency of 25%, a fill factor of about 83%, a short circuit current density of 43 mA/cm2, and an open circuit voltage of 0.706 V.
The perovskite solar cell also demonstrated improved stability during irradiation. While the reference perovskite cell devoid of MXene layers degraded within 10 minutes when exposed to 1 sun of irradiation, the complex perovskite/MXene sandwich cell retained 83% efficiency after 30 minutes of exposure. The researchers state 'The stabilization effect due to MXene can be related to the improved charge extinction, since trapped charges at the interfaces are known to trigger degradation.' Commercial stability standards requires less than 2-3% degradation in the first year, meaning additional research is necessary to address long-term perovskite cell stability even with MXene helper layers.
Density functional theory calculations supported these results, as calculated band profiles and Fermi levels matched well with those directly measured using ultraviolet photoelectron spectroscopy. Accounting for additional unexpected absorbance and an increased number of carriers within the calculations yielded excellent agreement and an appropriate model of MXene/perovskite interfacial interactions.
Using such a model and the supporting experimental results could help fine-tune future MXenes via surface modification to improve perovskite solar cell performance without mitigating or significantly altering other material properties.