5,769 research outputs found
Spin-orbit field switching of magnetization in ferromagnetic films with perpendicular anisotropy
As an alternative to conventional magnetic field, the effective spin-orbit
field in transition metals, derived from the Rashba field experienced by
itinerant electrons confined in a spatial inversion asymmetric plane through
the s-d exchange interaction, is proposed for the manipulation of
magnetization. Magnetization switching in ferromagnetic thin films with
perpendicular magnetocrystalline anisotropy can be achieved by current induced
spin-orbit field, with small in-plane applied magnetic field. Spin-orbit field
induced by current pulses as short as 10 ps can initiate ultrafast
magnetization switching effectively, with experimentally achievable current
densities. The whole switching process completes in about 100 ps.Comment: 4 pages, 3 figure
Magnetoplasmons excitations in graphene for filling factors
In the frame of the Hartree-Fock approximation, the dispersion of
magnetoplasmons in Graphene is derived for all types of transitions for filling
factors . The optical conductivity components of the magnetoplasmon
curves are calculated. It is shown that the electron-electron interactions lead
to a strong re-normalization of the apparent Fermi velocity of Graphene which
is different for different types of transitions.Comment: 15 pages, 7 figure
Double-exciton component of the cyclotron spin-flip mode in a quantum Hall ferromagnet
We report on the calculation of the cyclotron spin-flip excitation (CSFE) in
a spin-polarized quantum Hall system at unit filling. This mode has a
double-exciton component which contributes to the CSFE correlation energy but
can not be found by means of a mean field approach. The result is compared with
available experimental data.Comment: 9 pages, 2 figure
Robustness of Majorana Modes and Minigaps in a Spin-Orbit-Coupled Semiconductor-Superconductor Heterostructure
We study the robustness of Majorana zero energy modes and minigaps of
quasiparticle excitations in a vortex by numerically solving
Bogoliubov-deGennes equations in a heterostructure composed of an \textit{s}
-wave superconductor, a spin-orbit-coupled semiconductor thin film, and a
magnetic insulator. This heterostructure was proposed recently as a platform
for observing non-Abelian statistics and performing topological quantum
computation. The dependence of the Majorana zero energy states and the minigaps
on various physics parameters (Zeeman field, chemical potential, spin-orbit
coupling strength) is characterized. We find the minigaps depend strongly on
the spin-orbit coupling strength. In certain parameter region, the minigaps are
linearly proportional to the \textit{s}-wave superconducting pairing gap
, which is very different from the dependence in a
regular \textit{s-} or \textit{\p}-wave superconductor. We characterize the
zero energy chiral edge state at the boundary and calculate the STM signal in
the vortex core that shows a pronounced zero energy peak. We show that the
Majorana zero energy states are robust in the presence of various types of
impurities. We find the existence of impurity potential may increase the
minigaps and thus benefit topological quantum computation.Comment: 11 pages, 15 figure
Spin-Orbit Coupling and Tunneling Current in a Parabolic Quantum Dot
We propose a novel approach to explore the properties of a quantum dot in the
presence of the spin-orbit interaction and in a tilted magnetic field. The
spin-orbit coupling within the quantum dot manifest itself as anti-crossing of
the energy levels when the tilt angle is varied. The anti-crossing gap has a
non-monotonic dependence on the magnitude of the magnetic field and exhibits a
peak at some finite values of the magnetic field. From the dependence of the
tunneling current through the quantum dot on the bias voltage and the tilt
angle, the anti-crossing gap and most importantly the spin-orbit strength can
be uniquely determined
Interacting fermions in two dimensions: beyond the perturbation theory
We consider a system of 2D fermions with short-range interaction. A
straightforward perturbation theory is shown to be ill-defined even for an
infinitesimally weak interaction, as the perturbative series for the
self-energy diverges near the mass shell. We show that the divergences result
from the interaction of fermions with the zero-sound collective mode. By
re-summing the most divergent diagrams, we obtain a closed form of the
self-energy near the mass shell. The spectral function exhibits a threshold
feature at the onset of the emission of the zero-sound waves. We also show that
the interaction with the zero sound does not affect a non-analytic,
-part of the specific heat.Comment: 5 pages, 4 figure
About the global magnetic fields of stars
We present a review of observations of the stellar longitudinal (effective)
magnetic field () and its properties. This paper also discusses
contemporary views on the origin, evolution and structure of .Comment: Plenary report, The Gamov International Astronomical Conference, XIII
ODESSA, 19-25 August, 2013, Odessa, Ukrain
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