Equation of State of TiN at High Pressures and Temperatures: A Possible Host for Nitrogen in Planetary Mantles

1,2,3Daviau K.,1Fischer R.A.,1Brennan M.C.,1Dong J.,1Sure T.-A.,4Couper S.,5Meng Y.,6Prakapenka V.B.
Journal of Geophysical Research: Solid Earth 126, e2020JB020074 Link to Article [DOI
10.1029/2020JB020074]
1Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, United States
2Now at School of Science, University of Waikato, Tauranga, New Zealand
3Now at Toi-Ohomai Institute of Technology, Tauranga, New Zealand
4Department of Geology and Geophysics, University of Utah, Salt Lake City, UT, United States
5HPCAT, X-Ray Science Division, Argonne National Laboratory, Argonne, IL, United States
6Center for Advanced Radiation Sources, University of Chicago, Chicago, IL, United States

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One thought on “Equation of State of TiN at High Pressures and Temperatures: A Possible Host for Nitrogen in Planetary Mantles

  1. Pingback: Olivines in main-group pallasites: Magma-ocean cumulates or partial melting residues? | Cosmochemistry Papers

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