Solar thermochemical
ammonia (NH3) synthesis (STAS)
is a potential route to produce NH3 from air, water, and
concentrated sunlight. This process involves the chemical looping
of an active redox pair that cycles between a metal nitride and its
complementary metal oxide to yield NH3. To identify promising
candidates for STAS cycles, we performed a high-throughput thermodynamic
screening of 1,148 metal nitride/metal oxide pairs. This data-driven
screening was based on Gibbs energies of crystalline metal oxides
and nitrides at elevated temperatures, G(T), calculated using a recently introduced statistically
learned descriptor and 0 K DFT formation energies tabulated in the
Materials Project database. Using these predicted G(T) values, we assessed the viability of each of
the STAS reactionshydrolysis of the metal nitride, reduction
of the metal oxide, and nitrogen fixation to reform the metal nitrideand
analyzed a revised cycle that directly converts between metal oxides
and nitrides, which alters the thermodynamics of the STAS cycle. For
all 1148 redox pairs analyzed and each of the STAS-relevant reactions,
we implemented a Gibbs energy minimization scheme to predict the equilibrium
composition and yields of the STAS cycle, which reveals new active
materials based on B, V, Fe, and Ce that warrant further investigation
for their potential to mediate the STAS cycle. This work details a
high-throughput approach to assessing the relevant temperature-dependent
thermodynamics of thermochemical redox processes that leverages the
wealth of publicly available temperature-independent thermodynamic
data calculated using DFT. This approach is readily adaptable to discovering
optimal materials for targeted thermochemical applications and enabling
the predictive synthesis of new compounds using thermally controlled
solid-state reactions.