arXiv subjects

G. Chełkowska

Publications and source records attributed to G. Chełkowska.

4 recordsLinked to original sources

arXiv2025

Electronic structure of UGe$_2$ at ambient pressure: comparison with X-ray photoemission spectra

Based on experimental crystallographic data, electronic structure of UGe$_2$ have been calculated and compared with our results of X-ray photoelectron spectroscopy (XPS) measurements. We employed two different advanced full potential (FP) methods: FP-local-orbital (FPLO) and FP-linear augmented plane waves (Wien2k) codes for non-magnetic and ferromagnetic states. Starting from the local spin-density approximation (LSDA) or generalised gradient approximation (GGA), we verified either the orbital polarisation (OP) correction or the GGA+U approach for the U 5f-electrons, changing Coulomb-repulsion energies U in the range 0-4 eV. Satisfying agreement was achieved between experimental and our calculated magnetic moments using ab-initio LSDA+OP and non-ab-initio GGA+U approaches, the latter for realistic U values of 2-3 eV. We proved by the LSDA+OP approach an existence of the Fermi surface nesting vector along the a axis, possibly responsible for the triplet superconducting pairing. The calculated data reveal predominantly an itinerant U 5f-electron character of bands near the Fermi level, EF, with only small contributions from the U 6d and Ge 4p states. The experimental XPS spectrum of valence bands (VB) also contains the sharp main 5f-electron peak at EF, a wide hump (around -2 eV), and broad small peaks at higher energies. In the calculated XPS spectrum, the width of the main 5f-electron peak varies between 0.8 and 1.4 eV, depending on a method used in computations, but the hump remains unresolved. A newly observed asymmetric 1-eV satellite in the experimental 4f-core XPS spectrum together with known 3-eV and 7-eV satellites suggest dual behaviour of U-5f-electrons in UGe$_2$, the feature is inferred also from the VB studies.

cond-mat.mtrl-sci↗

arXiv2025

X-ray photoemission spectrum, electronic structure, and magnetism of UCu$_2$Si$_2$

The room temperature X-ray photoemission spectrum of the ferromagnetic compound UCu$_2$Si$_2$ (T$_C$ = 100 K) was measured using an Al K$_α$ source. Related theoretical spectra were computed from densities of electronic states obtained in the local density approximation (LDA), the generalized gradient approximation (GGA), and using the GGA+U method. The calculated spectrum is in a good agreement with the experimental one. The spin polarized calculations based on the GGA+U approach as well as GGA/LSDA with orbital polarization (OP) corrections taken into account provide values of the total magnetic moment in reasonable agreement with the experimental values ranging between 1.6 and 2.0 $μ_B$/U atom.

cond-mat.str-el↗

arXiv2025

Electronic structure of CeCo$_{1-x}$Fe$_x$Ge$_3$ studied by X-ray photoelectron spectroscopy and first-principles calculations

A transformation between the magnetically ordered CeCoGe$_3$ and heavy fermion CeFeGe$_3$ is isostructural but not isoelectronic, therefore the characterization of the electronic structure of the CeCo$_{1-x}$Fe$_x$Ge$_3$ series is of special importance. We report both the experimental investigation by the X-ray photoelectron spectroscopy (XPS) measurements and the first-principles calculations within the full-potential local-orbital (FPLO) scheme based on the density functional theory. Experimentally, we investigate mainly the valence band and the Ce $3d$ spectra, both giving the possibility to conclude about the level of the $f$ states localization. Computationally, we investigate the most characteristic CeCoGe$_3$, CeCo$_{0.5}$Fe$_{0.5}$Ge$_3$, and CeFeGe$_3$ compositions. Based on the electronic band structure results, we calculate the X-ray photoelectron spectra of the valence band. We consider the effects of the spin-orbit coupling and intra-atomic Hubbard U repulsion. Furthermore, we discuss the charge distribution and occupation of valence-band orbitals. The experimentally observed evolution of the 3$d$ band with the Fe concentration is related to the decrease of the number of electrons and reduction of the 3$d$ photoionization cross-sections. Calculations indicate that charge is transferred mainly from the Ce to Ge sites and the bondings are formed mainly by the Ce 5$d$, Fe/Co 3$d$, and Ge 4$p$ and 4$s$ orbitals.

cond-mat.mtrl-sci↗

arXiv2020

Influence of Pr substitution on physical properties of Ce$_{1-x}$Pr$_x$CoGe$_3$ system: A combined experimental and first-principles study

We present the results of our investigations of physical properties for the novel Ce$_{1-x}$Pr$_x$CoGe$_3$ system performed with a number of experimental methods: magnetic susceptibility, specific heat, electrical resistivity, magnetoresistance, and thermoelectric power. Moreover, the electronic structure was studied by means of photoelectron spectroscopy measurements and first-principles calculations. All investigated compositions of the Ce$_{1-x}$Pr$_x$CoGe$_3$ series crystallize in the tetragonal BaNiSn$_3$-type structure. The lattice parameters and unit cell volumes decrease with increasing Pr concentration. On the basis of the measurements taken, a preliminary magnetic phase diagram was created. A continuous suppression of the long-range magnetic ordering was observed with increase of Pr concentration. The critical Pr concentration for magnetic moment ordering was determined from linear extrapolation of the ordering temperature $versus$ $x$ to the lowest temperatures ($T = 0$ K) and is equal to about 0.66. Based on the first-principles calculations we show how the substitution of Pr for Ce affects the electronic structure and magnetic properties of the considered alloys. Within a single model we take into account the magnetic ordering, fully-relativistic effects, and Hubbard U repulsion on Ce and Pr. The impact of Hubbard U on the results of calculations is also discussed. We present the valence-band analysis, Mulliken electronic population analysis, and calculated electronic specific heat coefficients. For CeCoGe$_3$ it is found that the $++--$ configuration of magnetic moments on Ce is slightly more stable than the $+-+-$ one, and also that the calculated value of total magnetic moment on Ce (including spin and orbital parts) is in good agreement with the measurements.

cond-mat.str-el↗