28,547 research outputs found
Generalization of the effective Wiener-Ikehara theorem
International audienceWe consider the classical WienerâIkehara Tauberian theorem, with a generalized condition of slow decrease and some additional poles on the boundary of convergence of the Laplace transform. In this generality, we prove the otherwise known asymptotic evaluation of the transformed function, when the usual conditions of the Wiener-Ikehara theorem hold. However, our version also provides an effective error term, not known thus far in this generality. The crux of the proof is a proper asymptotic variation of the lemmas of Ganelius and Tenenbaum, also constructed for the sake of an effective version of the WienerâIkehara theorem
Pure braid subgroups of braided Thompson's groups
We describe pure braided versions of Thompson's group F. These groups,
and , are subgroups of the braided versions of Thompson's group V,
introduced by Brin and Dehornoy. Unlike V, elements of F are order-preserving
self-maps of the interval and we use pure braids together with elements of F
thus preserving order. We define these groups and give normal forms for
elements and describe infinite and finite presentations of these groups.Comment: 26 pages, 6 figures, with updated bibliograph
On one-dimensional models for hydrodynamics
To date it has not been possible to prove whether or not the
three-dimensional incompressible Euler equations develop singular behaviour in
finite time. Some possible singular scenarios, as for instance shock-waves, are
very important from a physical point of view, since they imply the connection
among the macroscopic and the microscopic scale. Therefore, the appearence of
this type of singularity or a similar one might be interpreted as a possible
explanation of the transition to turbulence. In order to clarify the question,
some one-dimensional models for ideal incompressible hydrodynamics have been
introduced and analyzed, and it was proven that shock-waves appear in finite
time within this type of flow. In this work we question the validity of these
models and analyze the physical meaning that the occurrence of a singularity in
an incompressible flow, if it happens, may have
The 2011 February superoutburst of the dwarf nova SDSS J112003.40+663632.4
We report unfiltered photometry of SDSS J112003.40+663632.4 during the 2011
February outburst which revealed the presence of superhumps with peak-to-peak
amplitude of up to 0.22 magnitudes showing this to be an SU UMa type dwarf
nova. The outburst amplitude was 5.4 magnitudes above mean quiescence and it
lasted at least 12 days. The mean superhump period during the plateau phase was
Psh = 0.07057(19) d.Comment: Accepted for publication in the Journal of the British Astronomical
Association. 12 pages, 5 figure
Detection of Supergranulation Alignment in Polar Regions of the Sun by Helioseismology
We report on a new phenomenon of `alignment' of supergranulation cells in the
polar regions of the Sun. Recent high-resolution datasets obtained by the Solar
Optical Telescope onboard the Hinode satellite enabled us to investigate
supergranular structures in high-latitude regions of the Sun. We have carried
out a local helioseismology time-distance analysis of the data, and detected
acoustic travel-time variations due to the supergranular flows. The
supergranulation cells in both the north and south polar regions show
systematic alignment patterns in the north-south direction. The south-pole
datasets obtained in a month-long Hinode campaign indicate that the
supergranulation alignment property may be quite common in the polar regions.
We also discuss the latitudinal dependence of the supergranulation cell sizes;
the data show that the east-west cell size decreases towards higher latitudes.Comment: 7 pages, 5 figures. Accepted for publication in ApJ Letters. Minor
modifications in figures and text
Magnetohydrodynamics of the Weakly Ionized Solar Photosphere
We investigate the importance of ambipolar diffusion and Hall currents for
high-resolution comprehensive ('realistic') photospheric simulations. To do so
we extended the radiative magnetohydrodynamics code \emph{MURaM} to use the
generalized Ohm's law under the assumption of local thermodynamic equilibrium.
We present test cases comparing analytical solutions with numerical simulations
for validation of the code. Furthermore, we carried out a number of numerical
experiments to investigate the impact of these neutral-ion effects in the
photosphere. We find that, at the spatial resolutions currently used (5-20 km
per grid point), the Hall currents and ambipolar diffusion begin to become
significant -- with flows of 100 m/s in sunspot light bridges, and changes of a
few percent in the thermodynamic structure of quiet-Sun magnetic features. The
magnitude of the effects is expected to increase rapidly as smaller-scale
variations are resolved by the simulations.Comment: accepted Ap
Negative powers of Laguerre operators
We study negative powers of Laguerre differential operators in , .
For these operators we prove two-weight estimates, with ranges of
depending on . The case of the harmonic oscillator (Hermite operator) has
recently been treated by Bongioanni and Torrea by using a straightforward
approach of kernel estimates. Here these results are applied in certain
Laguerre settings. The procedure is fairly direct for Laguerre function
expansions of Hermite type, due to some monotonicity properties of the kernels
involved. The case of Laguerre function expansions of convolution type is less
straightforward. For half-integer type indices we transfer the desired
results from the Hermite setting and then apply an interpolation argument based
on a device we call the {\sl convexity principle} to cover the continuous range
of . Finally, we investigate negative powers of the
Dunkl harmonic oscillator in the context of a finite reflection group acting on
and isomorphic to . The two weight estimates we
obtain in this setting are essentially consequences of those for Laguerre
function expansions of convolution type.Comment: 30 page
Emissions from pre-Hispanic metallurgy in the South American atmosphere
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