ﻻ يوجد ملخص باللغة العربية
We investigated theoretically electronic and magnetic properties of the perovskite material SrCoO$_{3-delta}$ with $deltaleq 0.15$ using a projector-augmented plane-wave method and a Greens function method. This material is known from various experiments to be ferromagnetic with a Curie temperature of 260$,$K to 305$,$K and a magnetic moment of 1.5${,mu_text{B}}$ to 3.0${,mu_text{B}}$. Applying the magnetic force theorem as it is formulated within Greens function method, we calculated for SrCoO$_{3-delta}$ the magnetic exchange parameters and estimated the Curie temperature. Including correlation effects by an effective $U$ parameter within the GGA$+U$ approach and verifying this by hybrid functional calculations, we obtained the Curie temperatures in dependence of the oxygen deficiency close to the experimental values.
It has been well established that both in bulk at ambient pressure and for films under modest strains, cubic SrCoO$_{3-delta}$ ($delta < 0.2$) is a ferromagnetic metal. Recent theoretical work, however, indicates that a magnetic phase transition to a
We present the first-principles investigation of the structural, electronic, and magnetic properties of SrCoO$_{3-delta}$ ($delta=0, 0.25, 0.5$) to understand the multivalent nature of Co ions in SrCoO$_{3-delta}$ along the line of topotactic transit
We studied structural, electronic and magnetic properties of a cubic perovskite BaFeO$_{3-delta}$ ($0 le delta le 0.5$) within the density functional theory using a generalized gradient approximation and a GGA+U method. According to our calculations,
Two magnetic phase transitions have been noted for SrCoO$_{3-y}$ for near-stoichiometric oxygen concentrations (small y). Using muon spin rotation and neutron scattering experiments, we have established that the two transitions represent separate, sp
Defects in semiconductors can exhibit multiple charge states, which can be used for charge storage applications. Here we consider such charge storage in a series of oxygen deficient phases of TiO$_2$, known as Magneli phases. These Ti$_n$O$_{2n-1}$ M