16,939 research outputs found
Photovoltaic effect in a gated two-dimensional electron gas in magnetic field
The photovoltaic effect induced by terahertz radiation in a gated
two-dimensional electron gas in magnetic field is considered theoretically. It
is assumed that the incoming radiation creates an ac voltage between the source
and gate and that the gate length is long compared to the damping length of
plasma waves. In the presence of pronounced Shubnikov-de Haas oscillations, an
important source of non-linearity is the oscillating dependence of the mobility
on the ac gate voltage. This results in a photoresponse oscillating as a
function of magnetic field, which is enhanced in the vicinity of the cyclotron
resonance, in accordance with recent experiments. Another, smooth component of
the photovoltage, unrelated to SdH oscillations, has a maximum at cyclotron
resonance.Comment: 4 pages, 3 figure
Recommended from our members
Characteristics and variability of storm tracks in the north Pacific, Bering Sea, and Alaska
The North Pacific and Bering Sea regions represent loci of cyclogenesis and storm track activity. In this paper climatological properties of extratropical storms in the North Pacific/Bering Sea are presented based upon aggregate statistics of individual storm tracks calculated by means of a feature-tracking algorithm run using NCEPâNCAR reanalysis data from 1948/49 to 2008, provided by the NOAA/Earth System Research Laboratory and the Cooperative Institute for Research in Environmental Sciences, Climate Diagnostics Center. Storm identification is based on the 850-hPa relative vorticity field (ζ) instead of the often-used mean sea level pressure; ζ is a prognostic field, a good indicator of synoptic-scale dynamics, and is directly related to the wind speed. Emphasis extends beyond winter to provide detailed consideration of all seasons.
Results show that the interseasonal variability is not as large during the spring and autumn seasons. Most of the storm variablesâgenesis, intensity, track densityâexhibited a maxima pattern that was oriented along a zonal axis. From season to season this axis underwent a northâsouth shift and, in some cases, a rotation to the northeast. This was determined to be a result of zonal heating variations and midtropospheric moisture patterns. Barotropic processes have an influence in shaping the downstream end of storm tracks and, together with the blocking influence of the coastal orography of northwest North America, result in high lysis concentrations, effectively making the Gulf of Alaska the âgraveyardâ of Pacific storms. Summer storms tended to be longest in duration. Temporal trends tended to be weak over the study area. SST did not emerge as a major cyclogenesis control in the Gulf of Alaska
GalPak3D: A Bayesian parametric tool for extracting morpho-kinematics of galaxies from 3D data
We present a method to constrain galaxy parameters directly from
three-dimensional data cubes. The algorithm compares directly the data with a
parametric model mapped in coordinates. It uses the spectral
lines-spread function (LSF) and the spatial point-spread function (PSF) to
generate a three-dimensional kernel whose characteristics are instrument
specific or user generated. The algorithm returns the intrinsic modeled
properties along with both an `intrinsic' model data cube and the modeled
galaxy convolved with the 3D-kernel. The algorithm uses a Markov Chain Monte
Carlo (MCMC) approach with a nontraditional proposal distribution in order to
efficiently probe the parameter space. We demonstrate the robustness of the
algorithm using 1728 mock galaxies and galaxies generated from hydrodynamical
simulations in various seeing conditions from 0.6" to 1.2". We find that the
algorithm can recover the morphological parameters (inclination, position
angle) to within 10% and the kinematic parameters (maximum rotation velocity)
to within 20%, irrespectively of the PSF in seeing (up to 1.2") provided that
the maximum signal-to-noise ratio (SNR) is greater than pixel
and that the ratio of the galaxy half-light radius to seeing radius is greater
than about 1.5. One can use such an algorithm to constrain simultaneously the
kinematics and morphological parameters of (nonmerging) galaxies observed in
nonoptimal seeing conditions. The algorithm can also be used on adaptive-optics
(AO) data or on high-quality, high-SNR data to look for nonaxisymmetric
structures in the residuals.Comment: 16 pages, 10 figures, accepted to publication in AJ, revised version
after proofs corrections. Algorithm available at http://galpak.irap.omp.e
Weierstrass's criterion and compact solitary waves
Weierstrass's theory is a standard qualitative tool for single degree of
freedom equations, used in classical mechanics and in many textbooks. In this
Brief Report we show how a simple generalization of this tool makes it possible
to identify some differential equations for which compact and even semicompact
traveling solitary waves exist. In the framework of continuum mechanics, these
differential equations correspond to bulk shear waves for a special class of
constitutive laws.Comment: 4 page
Dynamically-Induced Frustration as a Route to a Quantum Spin Ice State in Tb2Ti2O7 via Virtual Crystal Field Excitations and Quantum Many-Body Effects
The TbTiO pyrochlore magnetic material is attracting much
attention for its {\em spin liquid} state, failing to develop long range order
down to 50 mK despite a Curie-Weiss temperature K.
In this paper we reinvestigate the theoretical description of this material by
considering a quantum model of independent tetrahedra to describe its low
temperature properties. The naturally-tuned proximity of this system near a
N\'eel to spin ice phase boundary allows for a resurgence of quantum
fluctuation effects that lead to an important renormalization of its effective
low energy spin Hamiltonian. As a result, TbTiO is argued to be a
{\em quantum spin ice}. We put forward an experimental test of this proposal
using neutron scattering on a single crystal.Comment: 5 pages, 3 figures. Version 2 has a modified introduction. Figure 2b
of version 1 (experimental neutron scattering has been removed. A proposal
for an experimental test is now included accompanied by a new Figure (Fig. 3
- âŠ