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      Alkaline-earth metal (Mg) polynitrides at high pressure as possible high-energy materials

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          Abstract

          The P1̄-MgN 3 and P1̄-MgN 4 are predicted to become energetically stable under pressure, suggesting that it may be prepared by high-pressure synthesis. P1̄-MgN 3 and P1̄-MgN 4 are expected to release an enormously large amount of energy (2.83 and 2.01 kJ g −1). The present study encourages experimental exploration of these promising materials in the future.

          Abstract

          The high-pressure structural evolutionary behaviors of magnesium polynitrides were studied up to 100 GPa using first-principles calculations. Using the unbiased structure searching method, five stable chemical stoichiometries of magnesium polynitrides (MgN, Mg 2N 3, MgN 2, MgN 3, and MgN 4) were theoretically predicted at high pressures. The predicted MgN x compounds contain a rich variety of polynitrogen forms ranging from charged molecules (one-dimensional bent molecules N 3, planar triangle N 4 to benzene-like rings N 6) to extended polymeric chains (N ). To the best of our knowledge, this is the first time that stable bent molecules N 3, planar triangle N 4, and polymeric chains (N ) were predicted in alkaline-earth metal polynitrides. The decomposition of P1̄-MgN 3 and P1̄-MgN 4 are expected to be highly exothermic, releasing an energy of approximately 2.83 kJ g −1 and 2.01 kJ g −1, respectively. Furthermore, P1̄-MgN 4 can be synthesized at several GPa. The results of the present study suggest that it is possible to obtain energetic polynitrogen in main-group nitrides under high pressure.

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          Efficient iterative schemes forab initiototal-energy calculations using a plane-wave basis set

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            A simple measure of electron localization in atomic and molecular systems

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              Crystal structure prediction using ab initio evolutionary techniques: principles and applications.

              We have developed an efficient and reliable methodology for crystal structure prediction, merging ab initio total-energy calculations and a specifically devised evolutionary algorithm. This method allows one to predict the most stable crystal structure and a number of low-energy metastable structures for a given compound at any P-T conditions without requiring any experimental input. Extremely high (nearly 100%) success rate has been observed in a few tens of tests done so far, including ionic, covalent, metallic, and molecular structures with up to 40 atoms in the unit cell. We have been able to resolve some important problems in high-pressure crystallography and report a number of new high-pressure crystal structures (stable phases: epsilon-oxygen, new phase of sulphur, new metastable phases of carbon, sulphur and nitrogen, stable and metastable phases of CaCO3). Physical reasons for the success of this methodology are discussed.
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                Author and article information

                Journal
                PPCPFQ
                Physical Chemistry Chemical Physics
                Phys. Chem. Chem. Phys.
                Royal Society of Chemistry (RSC)
                1463-9076
                1463-9084
                2017
                2017
                : 19
                : 13
                : 9246-9252
                Affiliations
                [1 ]State Key Laboratory of Superhard Materials
                [2 ]College of Physics
                [3 ]Jilin University
                [4 ]Changchun
                [5 ]People's Republic of China
                Article
                10.1039/C6CP08771J
                34c1355e-3882-477c-ab4d-7420380e9c86
                © 2017
                History

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