7,576 research outputs found
Si/Ge hole-tunneling double-barrier resonant tunneling diodes formed on sputtered flat Ge layers
We have demonstrated Si/Ge hole-tunneling double-barrier resonant tunneling diodes (RTDs) formed on flat Ge layers with a relaxation rate of 89% by our proposed method; in this method, the flat Ge layers can be directly formed on highly B-doped Si(001) substrates using our proposed sputter epitaxy method. The RTDs exhibit clear negative differential resistance effects in the static currentâvoltage (IâV) curves at room temperature. The quantized energy level estimation suggests that resonance peaks that appeared in the IâV curves are attributed to hole tunneling through the first heavy- and light-hole energy levels
Imprint of Gravitational Lensing by Population III Stars in Gamma Ray Burst Light Curves
We propose a novel method to extract the imprint of gravitational lensing by
Pop III stars in the light curves of Gamma Ray Bursts (GRBs). Significant
portions of GRBs can originate in hypernovae of Pop III stars and be
gravitationally lensed by foreground Pop III stars or their remnants. If the
lens mass is on the order of and the lens redshift is
greater than 10, the time delay between two lensed images of a GRB is s and the image separation is as. Although it is difficult to
resolve the two lensed images spatially with current facilities, the light
curves of two images are superimposed with a delay of s. GRB light
curves usually exhibit noticeable variability, where each spike is less than
1s. If a GRB is lensed, all spikes are superimposed with the same time delay.
Hence, if the autocorrelation of light curve with changing time interval is
calculated, it should show the resonance at the time delay of lensed images.
Applying this autocorrelation method to GRB light curves which are archived as
the {\it BATSE} catalogue, we demonstrate that more than half light curves can
show the recognizable resonance, if they are lensed. Furthermore, in 1821 GRBs
we actually find one candidate of GRB lensed by a Pop III star, which may be
located at redshift 20-200. The present method is quite straightforward and
therefore provides an effective tool to search for Pop III stars at redshift
greater than 10. Using this method, we may find more candidates of GRBs lensed
by Pop III stars in the data by the {\it Swift} satellite.Comment: 13 pages, 13 figures, accepted for publication in Ap
Spin and interaction effects in quantum dots: a Hartree-Fock-Koopmans approach
We use a Hartree-Fock-Koopmans approach to study spin and interaction effects
in a diffusive or chaotic quantum dot. In particular, we derive the statistics
of the spacings between successive Coulomb-blockade peaks. We include
fluctuations of the matrix elements of the two-body screened interaction,
surface-charge potential, and confining potential to leading order in the
inverse Thouless conductance. The calculated peak-spacing distribution is
compared with experimental results.Comment: 5 pages, 4 eps figures, revise
Effects of carbon incorporation on doping state of YBa2Cu3Oy
Effects of carbon incorporation on the doping state of YBa2Cu3Oy (Y-123) were
investigated. Quantitative carbon analysis revealed that carbon could be
introduced into Y-123 from both the precursor and the sintering gas. Nearly
carbon-free (< 200 ppm) samples were prepared from a vacuum-treated precursor
by sintered at 900 ˚C and cooling with 20 ˚C /min in flowing oxygen
gas. The lower Tc (= 88 K) and higher oxygen content (y = 6.98) strongly
suggested the overdoping state, which was supported by the temperature
dependence of resisitivity and thermoelectric power. The nuclear quadrapole
resonance spectra and the Raman scattering spectra indicated that there was
almost no oxygen defect in the Cu-O chain in these samples. On the other hand,
in the same cooling condition, the samples sintered in air stayed at optimal
doping level with Tc = 93 K, and the intentionally carbon-doped sample was in
the underdoping state. It is revealed that about 60% of incorporated carbon was
substituted for Cu at the chain site in the form of CO32+, and the rest remains
at the grain boundary as carbonate impurities. Such incorporation affected the
oxygen absorption process in Y-123. It turned out that the oxygen content in
Y-123 cannot be controlled only by the annealing temperature and the oxygen
partial pressure but also by the incorporated carbon concentration.Comment: 16pages, 9figure
Effects of Specimen Size on Fatigue Property of Reduced Activation Ferritic/Martensitic Steel: JLF-1
Triaxial deformation in 10Be
The triaxial deformation in Be is investigated using a microscopic
model. The states of two valence neutrons are classified
based on the molecular-orbit (MO) model, and the -orbit is introduced
about the axis connecting the two -clusters for the description of the
rotational bands. There appear two rotational bands comprised mainly of and , respectively, at low excitation energy, where the two
valence neutrons occupy or orbits. The
triaxiality and the -mixing are discussed in connection to the molecular
structure, particularly, to the spin-orbit splitting. The extent of the
triaxial deformation is evaluated in terms of the electro-magnetic transition
matrix elements (Davydov-Filippov model, Q-invariant model), and density
distribution in the intrinsic frame. The obtained values turned out to be
.Comment: 15 pages, latex, 3 figure
Local moment formation in quantum point contacts
Spin-density-functional theory of quantum point contacts (QPCs) reveals the
formation of a local moment with a net of one electron spin in the vicinity of
the point contact - supporting the recent report of a Kondo effect in a QPC.
The hybridization of the local moment to the leads decreases as the QPC becomes
longer, while the onsite Coulomb-interaction energy remains almost constant.Comment: 10 pages, 3 figures, accepted for publication in Physical Review
Letter
Conductance Fluctuations in Disordered Wires with Perfectly Conducting Channels
We study conductance fluctuations in disordered quantum wires with unitary
symmetry focusing on the case in which the number of conducting channels in one
propagating direction is not equal to that in the opposite direction. We
consider disordered wires with left-moving channels and right-moving
channels. In this case, left-moving channels become perfectly conducting,
and the dimensionless conductance for the left-moving channels behaves as
in the long-wire limit. We obtain the variance of in the
diffusive regime by using the Dorokhov-Mello-Pereyra-Kumar equation for
transmission eigenvalues. It is shown that the universality of conductance
fluctuations breaks down for unless is very large.Comment: 6 pages, 2 figure
Distribution of Faraday Rotation Measure in Jets from Active Galactic Nuclei II. Prediction from our Sweeping Magnetic Twist Model for the Wiggled Parts of AGN Jets and Tails
Distributions of Faraday rotation measure (FRM) and the projected magnetic
field derived by a 3-dimensional simulation of MHD jets are investigated based
on our "sweeping magnetic twist model". FRM and Stokes parameters were
calculated to be compared with radio observations of large scale wiggled AGN
jets on kpc scales. We propose that the FRM distribution can be used to discuss
the 3-dimensional structure of magnetic field around jets and the validity of
existing theoretical models, together with the projected magnetic field derived
from Stokes parameters. In the previous paper, we investigated the basic
straight part of AGN jets by using the result of a 2-dimensional axisymmetric
simulation. The derived FRM distribution has a general tendency to have a
gradient across the jet axis, which is due to the toroidal component of the
magnetic field generated by the rotation of the accretion disk. In this paper,
we consider the wiggled structure of the AGN jets by using the result of a
3-dimensional simulation. Our numerical results show that the distributions of
FRM and the projected magnetic field have a clear correlation with the large
scale structure of the jet itself, namely, 3-dimensional helix. Distributions,
seeing the jet from a certain direction, show a good matching with those in a
part of 3C449 jet. This suggests that the jet has a helical structure and that
the magnetic field (especially the toroidal component) plays an important role
in the dynamics of the wiggle formation because it is due to a current-driven
helical kink instability in our model.Comment: Accepted for publication in Ap
- âŠ