TY - JOUR
T1 - Emergence of Novel Polynitrogen Molecule-like Species, Covalent Chains, and Layers in Magnesium-Nitrogen MgxNy Phases under High Pressure
AU - Yu, Shuyin
AU - Huang, Bowen
AU - Zeng, Qingfeng
AU - Oganov, Artem R.
AU - Zhang, Litong
AU - Frapper, Gilles
N1 - Publisher Copyright:
© 2017 American Chemical Society.
PY - 2017/6/1
Y1 - 2017/6/1
N2 - Stable structures and stoichiometries of binary Mg-N compounds are explored at pressures from ambient up to 300 GPa using ab initio evolutionary simulations. In addition to Mg3N2, we identified five nitrogen-rich compositions (MgN4, MgN3, MgN2, Mg2N3, and Mg5N7) and three magnesium-rich ones (Mg5N3, Mg4N3 and Mg5N4), which have stability fields on the phase diagram. These compounds have peculiar structural features, such as N2 dumbbells, bent N3 units, planar SO3-like N(N)3 units, N6 six-membered rings, 1D polythiazyl S2N2-like nitrogen chains, and 2D polymeric nitrogen nets. The dimensionality of the nitrogen network decreases as magnesium content increases; magnesium atoms act as a scissor by transferring valence electrons to the antibonding states of nitrogen sublattice. In this context, pressure acts as a bonding glue in the nitrogen sublattice, enabling the emergence of polynitrogen molecule-like species and nets. In general, Zintl-Klemm concept and molecular orbital analysis proved useful for rationalizing the structural, bonding and electronic properties encountered in the covalent nitrogen-based units. Interestingly, covalent six-membered N64- rings containing P-1 (I) MgN3 phase is recoverable at atmospheric pressure. Moreover, ab initio molecular dynamics analysis reveals the polymeric covalent nitrogen network, poly-N42-, encountered in the high-pressure Cmmm MgN4 phase can be preserved at ambient conditions. Thus, quenchable MgN4, stable at pressures above 13 GPa, shows that high energy-density materials based on polymeric nitrogen can be achievable at reduced pressures. The high-pressure phase P-1 (I) MgN3 with covalent N6 rings is the most promising HEDM candidate with an energy density of 2.87 kJ·g-1, followed by P-1 MgN4 (2.08 kJ·g-1).
AB - Stable structures and stoichiometries of binary Mg-N compounds are explored at pressures from ambient up to 300 GPa using ab initio evolutionary simulations. In addition to Mg3N2, we identified five nitrogen-rich compositions (MgN4, MgN3, MgN2, Mg2N3, and Mg5N7) and three magnesium-rich ones (Mg5N3, Mg4N3 and Mg5N4), which have stability fields on the phase diagram. These compounds have peculiar structural features, such as N2 dumbbells, bent N3 units, planar SO3-like N(N)3 units, N6 six-membered rings, 1D polythiazyl S2N2-like nitrogen chains, and 2D polymeric nitrogen nets. The dimensionality of the nitrogen network decreases as magnesium content increases; magnesium atoms act as a scissor by transferring valence electrons to the antibonding states of nitrogen sublattice. In this context, pressure acts as a bonding glue in the nitrogen sublattice, enabling the emergence of polynitrogen molecule-like species and nets. In general, Zintl-Klemm concept and molecular orbital analysis proved useful for rationalizing the structural, bonding and electronic properties encountered in the covalent nitrogen-based units. Interestingly, covalent six-membered N64- rings containing P-1 (I) MgN3 phase is recoverable at atmospheric pressure. Moreover, ab initio molecular dynamics analysis reveals the polymeric covalent nitrogen network, poly-N42-, encountered in the high-pressure Cmmm MgN4 phase can be preserved at ambient conditions. Thus, quenchable MgN4, stable at pressures above 13 GPa, shows that high energy-density materials based on polymeric nitrogen can be achievable at reduced pressures. The high-pressure phase P-1 (I) MgN3 with covalent N6 rings is the most promising HEDM candidate with an energy density of 2.87 kJ·g-1, followed by P-1 MgN4 (2.08 kJ·g-1).
UR - http://www.scopus.com/inward/record.url?scp=85020679898&partnerID=8YFLogxK
U2 - 10.1021/acs.jpcc.7b00474
DO - 10.1021/acs.jpcc.7b00474
M3 - 文章
AN - SCOPUS:85020679898
SN - 1932-7447
VL - 121
SP - 11037
EP - 11046
JO - Journal of Physical Chemistry C
JF - Journal of Physical Chemistry C
IS - 21
ER -