Sign Up to like & get recommendations! 1
Published in 2018 at "Applied Surface Science"
DOI: 10.1016/j.apsusc.2017.11.214
Abstract: Abstract Co2FeAl (CFA) films in a wide thickness range between 2 and 100 nm are sputtered at room temperature. Perpendicular magnetic anisotropy (PMA) is achieved in the annealed structure of Pd/CFA/MgO with CFA thickness ranging between… read more here.
Sign Up to like & get recommendations! 1
Published in 2018 at "Journal of Alloys and Compounds"
DOI: 10.1016/j.jallcom.2017.10.061
Abstract: Abstract The effects of Ge substitution and synthesis via rapid solidification on the structure and magnetic character of the intermetallic Fe 5 SiB 2 (5-1-2) system were determined, with the objective to investigate the potential… read more here.
Sign Up to like & get recommendations! 2
Published in 2017 at "Journal of Magnetism and Magnetic Materials"
DOI: 10.1016/j.jmmm.2017.05.059
Abstract: Abstract The behavior of local magnetic moments and exchange coupling parameters of Fe x Co 1 - x nanostructures (nanowires and compact clusters) on the fcc Pt(1 1 1) surface is here investigated using the first-principles real-space… read more here.
Sign Up to like & get recommendations! 1
Published in 2021 at "Journal of Magnetism and Magnetic Materials"
DOI: 10.1016/j.jmmm.2020.167483
Abstract: Abstract Effects of magnetic dipole interactions on specific loss power (SLP) for Zn0.3Fe2.7O4/SiO2 core/shell nanoparticles (NPs) with identical magnetic core size and varying non-magnetic shell thicknesses were systematically investigated. In the case of thin silica… read more here.
Sign Up to like & get recommendations! 0
Published in 2021 at "Journal of Magnetism and Magnetic Materials"
DOI: 10.1016/j.jmmm.2021.167780
Abstract: Abstract Multilayer planar nanostructures formed by ferromagnetic and heavy metals can reveal unique properties governed by their composition and geometry. The main role in their formation belongs to the interfacial spin-orbit interaction leading to specific… read more here.
Sign Up to like & get recommendations! 0
Published in 2017 at "RSC Advances"
DOI: 10.1039/c7ra01276d
Abstract: We reported an efficient way of preparing large and dense ferromagnetic arrays of vertically-aligned Ni nanotubes (NTs). The synthesis method allowed then for a direct, effective and controllable thermal conversion of the as-prepared Ni NTs… read more here.
Sign Up to like & get recommendations! 0
Published in 2019 at "New Journal of Chemistry"
DOI: 10.1039/c8nj04125c
Abstract: In this study, a novel core–shell structured nanocomposite of WO3 intermediate with LSPR was synthesized. This conclusion can solve the problems faced by magnetic–luminescent imaging materials and promote the application of this type of nanocomposites… read more here.
Sign Up to like & get recommendations! 0
Published in 2021 at "Chinese Physics B"
DOI: 10.1088/1674-1056/ac2252
Abstract: We would like to acknowledge the misprinted terms in our published paper “Simultaneous effects of magnetic field and space porosity on compressible Maxwell fluid transport induced by a surface acoustic wave in a microchannel” [Chin.… read more here.
Sign Up to like & get recommendations! 1
Published in 2017 at "Nuclear Fusion"
DOI: 10.1088/1741-4326/57/3/036009
Abstract: The effects of magnetic islands on electron bootstrap current in toroidal plasmas are studied using gyrokinetic simulations. The magnetic islands cause little changes of the bootstrap current level in the banana regime because of trapped… read more here.
Sign Up to like & get recommendations! 1
Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty154
Abstract: We present a large suite of simulations of the formation of low-mass star clusters. Our simulations include an extensive set of physical processes -- magnetohydrodynamics, radiative transfer, and protostellar outflows -- and span a wide… read more here.
Sign Up to like & get recommendations! 1
Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz2601
Abstract: The observed distribution of radii for exoplanets shows a bimodal form that can be explained by mass-loss from planetary atmospheres due to high-energy radiation emitted by their host stars. The location of the minimum of… read more here.