Abstract
Electronic and magnetic properties of , obtained from first-principles calculations employing the hybrid HSE06 functional, are presented for and 12.5% under pressures ranging from 0 to 15 GPa. In agreement with photoemission experiments at ambient pressure, we find for that nonhybridized Mn levels and Mn-induced states reside about 5 and 0.4 eV below the Fermi energy, respectively. For elevated pressures, the Mn levels, Mn-induced states, and the Fermi level shift toward higher energies, however the position of the Mn-induced states relative to the Fermi energy remains constant due to hybridization of the Mn levels with the valence As orbitals. We also evaluate, employing Monte Carlo simulations, the Curie temperature . At zero pressure, we obtain K, whereas the pressure-induced changes in are K/GPa for and an estimated value of K/GPa for under pressures up to 6 GPa. The determined values of compare favorably with –3) K/GPa at GPa found experimentally and estimated within the Zener model for in the regime where hole localization effects are of minor importance [M. Gryglas-Borysiewicz et al., Phys. Rev. B 82, 153204 (2010)].
- Received 24 February 2015
- Revised 27 April 2015
DOI:https://doi.org/10.1103/PhysRevB.91.184409
©2015 American Physical Society