1,459 research outputs found
Combining WASP and Kepler data: the case of the Sct star KIC 7106205
Ground-based photometric observations from Wide Angle Search for Planets (WASP) have been calibrated, scaled and combined with Kepler observations of the δ Sct star KIC 7106205, allowing us to extend the time base of the study of the unexplained amplitude and frequency variation of a single pressure mode at ν = 13.3942 d−1 by 2 yr. Analysis of the combined data sets, spanning 6 yr, show that the amplitude modulation in KIC 7106205 has a much larger range than a previous study of the Kepler data alone indicated. The single pressure mode decreased from 11.70 ± 0.05 mmag in 2007, to 5.87 ± 0.03 mmag in 2009, and to 0.58 ± 0.06 mmag in 2013. Observations of the decrease in mode amplitude have now been extended back 2 yr before the launch of Kepler. With observations over a longer time span, we have been able to further investigate the decrease in mode amplitude in KIC 7106205 to address the question of mode amplitude stability in δ Sct stars. This study highlights the usefulness of the WASP data set for extending studies of some Kepler variable stars
Criterion for universality class independent critical fluctuations: example of the 2D Ising model
Order parameter fluctuations for the two dimensional Ising model in the
region of the critical temperature are presented. A locus of temperatures T*(L)
and of magnetic fields B*(L) are identified, for which the probability density
function is similar to that for the 2D-XY model in the spin wave
approximation.The characteristics of the fluctuations along these points are
largely independent of universality class. We show that the largest range of
fluctuations relative to the variance of the distribution occurs along these
loci of points, rather than at the critical temperature itself and we discuss
this observation in terms of intermittency. Our motivation is the
identification of a generic form for fluctuations in correlated systems in
accordance with recent experimental and numerical observations. We conclude
that a universality class dependent form for the fluctuations is a
particularity of critical phenomena related to the change in symmetry at a
phase transition.Comment: to appear in Phys. Rev.
Intermittency and non-Gaussian fluctuations of the global energy transfer in fully developed turbulence
We address the experimentally observed non-Gaussian fluctuations for the
energy injected into a closed turbulent flow at fixed Reynolds number. We
propose that the power fluctuations mirror the internal kinetic energy
fluctuations. Using a stochastic cascade model, we construct the excess kinetic
energy as the sum over the energy transfers at different levels of the cascade.
We find an asymmetric distribution that strongly resembles the experimental
data. The asymmetry is an explicit consequence of intermittency and the global
measure is dominated by small scale events correlated over the entire system.
Our calculation is consistent with the statistical analogy recently made
between a confined turbulent flow and a critical system of finite size.Comment: To appear in Physical Review Letter
Nature of finite-temperature transition in anisotropic pyrochlore Er2Ti2O7
We study the finite-temperature transition in a model XY antiferromagnet on a
pyrochlore lattice, which describes the pyrochlore material Er2Ti2O7. The
ordered magnetic structure selected by thermal fluctuations is six-fold
degenerate. Nevertheless, our classical Monte Carlo simulations show that the
critical behavior corresponds to the three-dimensional XY universality class.
We determine an additional critical exponent nu_6=0.75>nu characteristic of a
dangerously irrelevant scaling variable. Persistent thermal fluctuations in the
ordered phase are revealed in Monte Carlo simulations by the peculiar
coexistence of Bragg peaks and diffuse magnetic scattering, the feature also
observed in neutron diffraction experiments.Comment: 5+5 pages (including supplemental material
THE RELATION OF THE EQUITY ADMINISTERED BY THE COMMON LAW JUDGES TO THE EQUITY ADMINISTERED BY THE CHANCELLOR
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