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Explore BSCF type cathodes for solid oxide fuel cells via large-scale computer simulations in materials science. Conduct advanced theoretical modeling using DFT methods.
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First principles calculations of BSCF material for membrane applications Eugene Kotomin Laboratory of Theoretical Physics and Computer Simulations of materials NASA Meeting
One of main priorities of our laboratory: New/more efficient Energy Sources and New Materials for energy applications1. advanced nuclear fuels for Generation IV reactors2. New construction reactor (radiation resistant) materials 3. solid oxide fuel cells: 80% conversion of chemical energy into electricity4. Ceramic membranes NASA Meeting
Development of new materials • Large scale computer simulations of materials in close collaboration with state-of-the art experiments [Max Planck Institute, Stuttgart]: Try-and-error approach does not work! Limitations of experiments: Discrimination of processes (O vacancies migration) in the bulk and on surfaces, A role of different dopands and impurities Identification of adsorbates at low coverages NASA Meeting
General problem Improvement of SOFC and membrane performance requires -- better understanding of Study and control of possible reaction pathways of oxygen reduction and incorporation reaction • Exciting and challenging multidisciplinary field: • Electrochemistry and materials chemistry, • surface science of advanced oxides, • , chemical kinetics, • large-scale computer simulations NASA Meeting
Materials of interest: magnetic perovskites • LaMnO3 (LMO) – model material • La1-xSrxMnO3 (LSM)– real cathode material • Multi-component BSCF type cathodes These strongly correlated materials reveal numerous phenomena due to a combination of spin, orbit, lattice degrees of freedom -- 2 areas of applications: low-T (spintronics) -- high T: solid oxide fuel cells NASA Meeting
First experience with theoretical modelling of LSM: • E.Kotomin et al, PCCP 10, 4644 (2008) • R.Merkle et al, J. ECS Trans. 25, 2753 (2009) • Yu.Mastrikov et al. J Phys Chem. C, 114, 3017 2010. • First BSCF paper submitted to Enenrgy and Environmental Science, 2010. Standard DFT (GGA) or DFT-HF hybrids calculations of large, low symmetry systems with defects and surfaces (up to 320 atoms per supercell) NASA Meeting
Method Density Functional Theory Plane Wave basis set 4.6.19 08Dec03, Georg Kresse and Jürgen Furthmüller Institut für Materialphysik, Universität Wien Generalised Gradient Approximation Perdew Wang 91 exchange-correlation functional Projector Augmented Wave method Davidson algorithm for electronic optimization Conjugate Gradient method for structure relaxation Nudged Elastic Bands for energy barriers estimation Badercharge analysis (Prof. G. Henkelmanand co-workers, Universiy of Texas) NASA Meeting
Computational detailsVASP: GGA PW calculations • atoms description: • kinetic energy cutoff: 400 eV > Ecutmax = 269.887 eV • Monkhorst-Pack k-points sampling < 0.27 Å-1 NASA Meeting
La Mn O Test calculations(PCCP 7, 2346 (2005) Bulk calculations Surface calculations Orthorhombic (Pbnm) (001) (110) (111) a b c Structure optimisation for the FM,A-, C-, G-AF and non-magnetic states • Cohesive energy, Structure,ionic charges • practically (<1%) do not depend on • the specific magnetic ordering • In a good agreement with experimental data • Non-magnetic state – very unfavourable • High covalency of the Mn-O bonding 7-, 8-plane slabs are sufficiently thick for surface processes modelling Spin-polarized calculations Charges on the two surface planes are not affected by slab stoichiometry NASA Meeting
Preliminary results:Ba(0.5)Sr(0.5)Co(0.75)Fe(0.25)O3-δ Ba Co Sr Fe O Bulk and defect properties 40 atom supercells (12.5%) and 320 atoms (1.5%) NASA Meeting
Test: pure ABO3 perovskites Lattice constants (A, cubic phase) A B Co* Fe** Ba 3.96(--) 3.97(4.04) Sr 3.84(3.83) 3.85(3.85) *IS, **HS Pure BSCF: a_o=3.90-3.92 A (expt 3.98A) NASA Meeting
Effective (static) Bader atomic charges,e Ba, Sr 1.57e close to formal +2e Co 1.71e Fe 1.88e O -1.1 e Strong covalent contribution to the bonding NASA Meeting
Co-Vo-Fe vacancy NASA Meeting
Vacancy formation energies • (Ba,Sr)CoO3 ca. 1 eV (LaCoO3 1.5 eV) • (Ba,Sr)FeO3 ca. 2.4 eV (LaFeO3 1.2 eV) • LMO 4.5-5 eV expt 3 eV • STO 5.5-6 eV expt 5 eV Charge disproportionation effect: 2Fe(3+)=Fe(2+) + Fe (4+) is neglected in theory NASA Meeting
Charge redistribution around Vo Red is electronic density deficiency, blue- excess Charge of a missing O2- ion is spread over nearest Co and Fe ions NASA Meeting
Calculated lattice constants Incorporation of vacancies improves agreement with the experiment Oxygen deficiency, NASA Meeting
Vacancy migration energy 0.46 eV Co-Vo-Fe Co-Vo-Co 0.46 eV Co-Vo-Fe 0.52 eV Co-Vo-Co 0.42 eV For comparison: LMO 0.9 eV NASA Meeting
Our ultimate goal:--the mechanism of the oxygenreduction in different materials [LSCF?] under different conditions,--understanding of the limiting reaction steps,--increase of O reduction efficiency NASA Meeting
Milestones:Atomistic/mechanistic details hardly detectable experimentally:-- Optimal sites for oxygen adsorption-- the energetics of O2 dissociation,-- O and vacancy migration on the surface -- O penetration to cathode surface: what are the rate-determining reaction stages, O diffusion NASA Meeting
Mechanism of oxygen reduction M2 in LSM (Merkle et al, J ECS Trans.2009) NASA Meeting
3 possible mechanisms of oxygen incorporation --The rate-determining step is encounter of adsorbed molecular oxygen (superoxide O2- or peroxide O2 (2-) )with a surface oxygen vacancy --Both vacancy concentration and mobility are important for a fast oxygen Incorporation NASA Meeting
3 possible mechanisms for oxygen reduction on LSM NASA Meeting
Thermodynamics of the O adsorption at different temperatures and O2 gas pressures NASA Meeting
Conclusions • Standard ab initio computer codes are able to shed some additional light on cathode/surface reactions where expt tools are of a limited applicability • We reproduce Vo low migration energies • Lattice structure role of structural Vo • low Vo formation energies • To be used in the analysis of BSCF cathode/membrane performance NASA Meeting