Ab Initio Calculations of Phase Stability in the N–H System at Pressures up to 1.5 TPa

The stability of compounds in the N–H system at 0 K to pressures of 1.5 TPa has been calculated. The evolutionary search for stable structures in the USPEX program has been carried out using the PBEsol + vdW method within the density functional theory. New stable structures in the NH and N3H10 compounds have been discovered and the boundaries of phase transitions in the N3H7, NH3, and NH4 compounds have been refined. At a maximum pressure of 1.5 TPa, stable phases are NH with the P4122 and P4322 structures and NH4 with the C2/c structure. The obtained data can be used for the subsequent calculation of the equations of state of the phases of the N–H system, which is important for planetary physics.

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Publication Details

Journal
Journal of Experimental and Theoretical Physics Letters
Published
2025-12-01
DOI
https://doi.org/10.1134/s0021364025609285
Primary Topic
High-pressure geophysics and materials
Type
article
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article

Ab Initio Calculations of Phase Stability in the N–H System at Pressures up to 1.5 TPa

V. V. Brazhkin, K. D. Litasov, T. M. Inerbaev, N. E. Sagatov
Journal of Experimental and Theoretical Physics Letters
High-pressure geophysics and materials
article

Ab Initio Calculations of Phase Stability in the N–H System at Pressures up to 1.5 TPa

V. V. Brazhkin, K. D. Litasov, T. M. Inerbaev, N. E. Sagatov
article en

Abstract

The stability of compounds in the N–H system at 0 K to pressures of 1.5 TPa has been calculated. The evolutionary search for stable structures in the USPEX program has been carried out using the PBEsol + vdW method within the density functional theory. New stable structures in the NH and N3H10 compounds have been discovered and the boundaries of phase transitions in the N3H7, NH3, and NH4 compounds have been refined. At a maximum pressure of 1.5 TPa, stable phases are NH with the P4122 and P4322 structures and NH4 with the C2/c structure. The obtained data can be used for the subsequent calculation of the equations of state of the phases of the N–H system, which is important for planetary physics.

Journal of Experimental and Theoretical Physics LettersVol. 122(12)
L. N. Gumilyov Eurasian National University (KZ), Russian Academy of Sciences (RU), Institute for High Pressure Physics (RU), V.I. Vernadsky Institute of Geochemistry and Analytical Chemistry (RU)
Openalex Percentile: Top 25%
High-pressure geophysics and materials
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