Published June 7, 2019 | Version Accepted Version + Supplemental Material
Journal Article Open

Reaction mechanism and kinetics for ammonia synthesis on the Fe(211) reconstructed surface

  • 1. ROR icon University of Nevada Reno
  • 2. ROR icon California Institute of Technology
  • 3. ROR icon National Research Council

Abstract

To provide guidelines to accelerate the Haber–Bosch (HB) process for synthesis of ammonia from hydrogen and nitrogen, we used Quantum Mechanics (QM) to determine the reaction mechanism and free energy reaction barriers under experimental reaction conditions (400 °C and 20 atm) for all 10 important surface reactions on the Fe(211) reconstructed (Fe(211)R) surface. These conditions were then used in full kMC modeling for 30 minutes to attain steady state. We find that the stable surface under Haber–Bosch conditions is the missing row 2 × 1 reconstructed surface (211)R and that the Turn Over Frequency (TOF) is 18.7 s^(−1) per 2 × 2 surface site for 1.5 Torr NH_3 pressure, but changes to 3.5 s^(−1) for 1 atm, values close (within 6%) to the ones on Fe(111). The experimental ratio between (211) and (111) rates at low (undisclosed) NH_3 pressure was reported to be 0.75. The excellent agreement with experiment on two very different surfaces and reaction mechanisms is a testament of the accuracy of QM modeling. In addition, our kinetic analysis indicates that Fe(211)R is more active than Fe(111) at high pressure, close to HB industrial conditions, and that (211)R is more abundant than (111) via a steady-state Wulff construction under HB conditions. Thus, at variance with common thinking, we advocate the Fe(211)R surface as the catalytically active phase of pure iron ammonia synthesis catalyst under HB industrial conditions.

Additional Information

© 2019 the Owner Societies. Received 22nd March 2019, Accepted 14th May 2019, First published on 14th May 2019. This work was supported by the U.S. Department of Energy (USDOE), Office of Energy Efficiency and Renewable Energy (EERE), Advanced Manufacturing Office Next Generation R&D Projects under contract no. DE-AC07-05ID14517 (program manager Dickson Ozokwelu, in collaboration with Idaho National Laboratories, Rebecca Fushimi). A. F. gratefully acknowledges financial support from a Short-Term Mission (STM) funded by Italian Consiglio Nazionale delle Ricerche (CNR). We would like to thank the Information Technology department at the University of Nevada, Reno for computing time on the High Performance Computing Cluster (Pronghorn). Some calculations were also carried out on a GPU-cluster provided by DURIP (Cliff Bedford, program manager). Authors contributions: AF, WAG and QA designed the strategy of this work. JF and QA performed QM calculations. AF performed kMC simulations. All authors wrote the paper. The authors declare no competing financial interest.

Attached Files

Accepted Version - 1336-Fe_211_HaberBosch.pdf

Supplemental Material - c9cp01611b1_si.pdf

Supplemental Material - c9cp01611b2_si.xlsx

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Additional details

Identifiers

Eprint ID
95642
DOI
10.1039/c9cp01611b
Resolver ID
CaltechAUTHORS:20190521-110908971

Related works

Describes
10.1039/c9cp01611b (DOI)

Funding

Department of Energy (DOE)
DE-AC07-05ID14517
Consiglio Nazionale delle Ricerche (CNR)

Dates

Created
2019-05-21
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Astronomy Department
Other Numbering System Name
WAG
Other Numbering System Identifier
1336