675 research outputs found
Longitudinal and transverse noise in a moving Vortex Lattice
We have studied the longitudinal and the transverse velocity fluctuations of
a moving vortex lattice (VL) driven by a transport current. They exhibit both
the same broad spectrum and the same order of magnitude. These two components
are insensitive to the velocity and to a small bulk perturbation. This means
that no bulk averaging over the disorder and no VL crystallization are
observed. This is consistently explained referring to a previously proposed
noisy flow of surface current whose elementary fluctuator is measured
isotropic.Comment: accepted for publication in Phys Rev
Stochastic excitation of non-radial modes I. High-angular-degree p modes
Turbulent motions in stellar convection zones generate acoustic energy, part
of which is then supplied to normal modes of the star. Their amplitudes result
from a balance between the efficiencies of excitation and damping processes in
the convection zones. We develop a formalism that provides the excitation rates
of non-radial global modes excited by turbulent convection. As a first
application, we estimate the impact of non-radial effects on excitation rates
and amplitudes of high-angular-degree modes which are observed on the Sun. A
model of stochastic excitation by turbulent convection has been developed to
compute the excitation rates, and it has been successfully applied to solar
radial modes (Samadi & Goupil 2001, Belkacem et al. 2006b). We generalize this
approach to the case of non-radial global modes. This enables us to estimate
the energy supplied to high-() acoustic modes. Qualitative arguments as
well as numerical calculations are used to illustrate the results. We find that
non-radial effects for modes are non-negligible:
- for high- modes (i.e. typically ) and for high values of ;
the power supplied to the oscillations depends on the mode inertia.
- for low- modes, independent of the value of , the excitation is
dominated by the non-diagonal components of the Reynolds stress term. We
carried out a numerical investigation of high- modes and we find that
the validity of the present formalism is limited to due to the
spatial separation of scale assumption. Thus, a model for very high-
-mode excitation rates calls for further theoretical developments, however
the formalism is valid for solar modes, which will be investigated in a
paper in preparation.Comment: 12 pages, accepted for publication in A&
Chikungunya Virus Infection-Associated Bone and Joint Disease
Chikungunya virus (CHIKV) is a mosquito-borne alphavirus that circulates predominantly in tropical and subtropical regions. Infection results in severe debilitating polyarthralgia during the acute phase of disease, and reports suggest that chronic arthralgia lasting months to years after the initial infection can occur. More severe and prolonged disease has been associated with pre-existing joint disease, though this has not been experimentally examined. In the research presented herein, two established mouse models (adult IRF 3/7 -/- -/- and wild-type C57BL/6J mice) were utilized to characterize CHIKV-associated bone and joint disease and evaluate its impact on the progression of pre-existing osteoarthritis (OA) utilizing histopathology, μCT, and serology. During acute stages of the disease, CHIKV infection resulted in synovitis, cartilage necrosis, and periosteal necrosis or periostitis. Additionally, IRF mice had severe ischemic bone marrow necrosis, and C57BL/6J mice developed periosteal new bone proliferation. During chronic stages of disease (90 DPI), there was ongoing and progressive synovitis, tendonitis, enthesitis, and cartilage damage, though periostitis and periosteal bone proliferation had resolved. Infection with CHIKV in mice with pre-existing OA had no significant impact on total synovitis scores or chondrocyte cell death, but caused a decrease in volume of osteophytes and subchondral bone, as compared to OA alone. Serology results in both the footpad and intra-articular C57BL/6J models indicated there were alterations in RANKL and OPG associated with CHIKV infection, demonstrating potential changes in bone dynamics. The current experiments demonstrated novel lesions of CHIKV-associated bone and joint disease that have important ramifications for the treatment and prevention of disease. Periosteal bone proliferation associated with CHIKV is a potentially painful but reversible process, whereas articular cartilage damage is progressive and represents a potential mechanism for chronic CHIKV-associated joint disease. Additionally, the alterations in bone associated with CHIKV infection and pre-existing OA, in conjunction with changes in the RANKL-OPG pathways, could have significance in clinical monitoring of OA and treatment choices in individuals with concurrent diseases. Future studies would help determine if RANKL and OPG levels could be useful for tracking disease progression in people and establish the long-term effects of CHIKV infection on OA progression
Electrodynamics of the vortex lattice in untwinned YBaCuO by complex impedance measurements
We report complex impedance measurements in an untwinned YBaCuO crystal. Our
broad frequency range covers both the quasi static response and the resistive
response of the vortex lattice. It allow us to characterize the irreversibility
line without the need of any frequency dependent pinning parameters. We confirm
the validity of the two modes model of vortex dynamic, and extract both the
surface critical current and the flux flow resistivity around the first order
transition . This latter is identified by the abrupt loss of pinning and
by an unexpected step of at .Comment: accepted for publication in EPJ
Numerical constraints on the model of stochastic excitation of solar-type oscillations
Analyses of a 3D simulation of the upper layers of a solar convective
envelope provide constraints on the physical quantities which enter the
theoretical formulation of a stochastic excitation model of solar p modes, for
instance the convective velocities and the turbulent kinetic energy spectrum.
These constraints are then used to compute the acoustic excitation rate for
solar p modes, P. The resulting values are found ~5 times larger than the
values resulting from a computation in which convective velocities and entropy
fluctuations are obtained with a 1D solar envelope model built with the
time-dependent, nonlocal Gough (1977) extension of the mixing length
formulation for convection (GMLT). This difference is mainly due to the assumed
mean anisotropy properties of the velocity field in the excitation region. The
3D simulation suggests much larger horizontal velocities compared to vertical
ones than in the 1D GMLT solar model. The values of P obtained with the 3D
simulation constraints however are still too small compared with the values
inferred from solar observations. Improvements in the description of the
turbulent kinetic energy spectrum and its depth dependence yield further
increased theoretical values of P which bring them closer to the observations.
It is also found that the source of excitation arising from the advection of
the turbulent fluctuations of entropy by the turbulent movements contributes ~
65-75 % to the excitation and therefore remains dominant over the Reynolds
stress contribution. The derived theoretical values of P obtained with the 3D
simulation constraints remain smaller by a factor ~3 compared with the solar
observations. This shows that the stochastic excitation model still needs to be
improved.Comment: 11 pages, 9 figures, accepted for publication in A&
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