Recent discoveries in high-pressure chemistry have revealed
a greater
richness in the interaction between transition metals and nitrogen,
particularly with the synthesis of various metal nitrides. In this
study, we investigate novel Sr–N phases under varying moderate
pressures, employing evolutionary algorithms (EAs) and based on first-principles
calculations to explore their thermodynamic, structural, and electronic
characteristics. Our comprehensive analysis includes assessments of
thermodynamic stability based on convex hulls and confirmation of
dynamical stability through phonon calculations. Through these analyses,
we identify four stable structuresSrN, SrN2, SrN3, and SrN4along with their corresponding
pressure-induced structures presented in a phase diagram. Electronic
band structure calculations offer insights into the electronic behaviors
of these phases under different pressures. Notably, in the cases of
SrN3 and SrN4, the high PDOS at the Fermi energy
suggests the potential for superconductivity (SC) in these phases.
Furthermore, our study unveils the superconducting behavior of SrN4 within the pressure range of 10–50 GPa, with a peak T
c reaching 13.7 K at 10 GPa. This observation
reflects an enhancement of T
c under pressure,
attributed to the introduction of nitrogen. These findings provide
valuable insights into the diverse Sr–N phases under pressure
obtained from evolutionary algorithms and predict the possibility
of SC in certain phases, opening avenues for further exploration in
metal nitrides under pressures.