In this study, we investigated the effect of infiltrated material and nitrate concentration used for sol-impregnation process on the resulting kinetics and rate-limiting steps of ORR. Various infiltrates were chosen based upon the specific merits of each material in terms of electronic/ionic conductivity, oxygen exchange activity and oxygen storage capability. The infiltrates of study includes LaxSr1-xCoyFe1-yO3-δ (LSCF), La1-xSrxMnO3-δ (LSM), Gd1-xCexO2-δ (GDC), Sm1-xCexO3-δ (SDC), Pr1-xCexO3-δ (PDC), Pr6O11 and LaNi1-xFexO3-δ (LNF). Porous LNF was used as the cathodic backbone. For each infiltrate type, sols with different molar concentrations ranging from 0.2 M to 5.0 M were applied for the infiltration process. For every infiltration process, only one infiltration process was performed without a separate sintering/annealing step.
Results showed that an infiltration even with LNF, the same material with the backbone reduced the cathodic polarization resistance (Rp) from 2.6 (bare LNF) to 0.15 W cm2 at 700 °C, indicating the critical importance of active surface area for cathodic performance in this system. Infiltration with 1.0 M of Pr6O11 rendered the best performance (Rp = 0.055 W cm2 at 700 °C). With a concentration of 1.0 M or higher, the infiltrate comprises > 20 wt.%, a concentration high enough to infiltrate Pr6O11 throughout the surface of LNF backbone uniformly as observed by electron microscope images. The activation energy of cathodic polarization decreased from 1.75 eV (bare LNF) to 1.0 – 1.2 eV (1.12 eV for 1 M LNF; 1.18 eV for 1 M Pr6O11, 1.06 eV for 1 M LSCF), indicating a shift in the rate limiting step by the infiltration. There was, however, little dependency of activation energy on the molar concentration in a given infiltrate material as long as the concentration is > ~0.5 M. In addition, the dependency on oxygen partial pressure also provided critical clues on the shift in the rate-limiting steps of ORR, and relevant discussion will be provided in the presentation.
This work was supported by the NASA MIRO Program (NNX15AQ01A).
References
[1] D. Ding, X. Li, S. Y. Lai, K. Gerdes, M. Liu, Energy Environ. Sci. 2014, 7, 552.