1,728 research outputs found
Accurate control of a Bose-Einstein condensate by managing the atomic interaction
We exploit the variation of the atomic interaction in order to move
ultra-cold atoms across an AC-driven periodic lattice. By breaking relevant
symmetries, a gathering of atoms is achieved. Accurate control of the gathered
atoms positions can be demonstrated via the control of the atomic localization
process. The localization process is analyzed with the help of the nonlinear
Floquet states where the Landau-Zener tunneling between states is observed and
controlled. Transport effects in the presence of disorder are discussed.Comment: 14 pages, 5 Figures, PACS numbers: 03.75.Lm, 05.60.-k, 63.20.P
Soliton dynamics in damped and forced Boussinesq equations
We investigate the dynamics of a lattice soliton on a monatomic chain in the
presence of damping and external forces. We consider Stokes and hydrodynamical
damping. In the quasi-continuum limit the discrete system leads to a damped and
forced Boussinesq equation. By using a multiple-scale perturbation expansion up
to second order in the framework of the quasi-continuum approach we derive a
general expression for the first-order velocity correction which improves
previous results. We compare the soliton position and shape predicted by the
theory with simulations carried out on the level of the monatomic chain system
as well as on the level of the quasi-continuum limit system. For this purpose
we restrict ourselves to specific examples, namely potentials with cubic and
quartic anharmonicities as well as the truncated Morse potential, without
taking into account external forces. For both types of damping we find a good
agreement with the numerical simulations both for the soliton position and for
the tail which appears at the rear of the soliton. Moreover we clarify why the
quasi-continuum approximation is better in the hydrodynamical damping case than
in the Stokes damping case
Time-frequency analysis of the restricted three-body problem: transport and resonance transitions
A method of time-frequency analysis based on wavelets is applied to the problem of transport between different regions of the solar system, using the model of the circular restricted three-body problem in both the planar and the spatial versions of the problem.. The method is based on the extraction of instantaneous frequencies from the wavelet transform of numerical solutions. Time-varying frequencies provide a good diagnostic tool to discern chaotic trajectories from regular ones, and we can identify resonance islands that greatly affect the dynamics. Good accuracy in the calculation of time-varying frequencies allows us to determine resonance trappings of chaotic trajectories and resonance transitions. We show the relation between resonance transitions and transport in different regions of the phase space
The Energy-dependent X-ray Timing Characteristics of the Narrow Line Seyfert 1 Mkn 766
We present the energy-dependent power spectral density (PSD) and
cross-spectral properties of Mkn 766, obtained from combining data obtained
during an XMM-Newton observation spanning six revolutions in 2005 with data
obtained from an XMM-Newton long-look in 2001. The PSD shapes and rms-flux
relations are found to be consistent between the 2001 and 2005 observations,
suggesting the 2005 observation is simply a low-flux extension of the 2001
observation and permitting us to combine the two data sets. The resulting PSD
has the highest temporal frequency resolution for any AGN PSD measured to date.
Applying a broken power-law model yields break frequencies which increase in
temporal frequency with photon energy. Obtaining a good fit when assuming
energy-independent break frequencies requires the presence of a Lorentzian at
4.6+/-0.4 * 10^-4 Hz whose strength increases with photon energy, a behavior
seen in black hole X-ray binaries. The cross-spectral properties are measured;
temporal frequency-dependent soft-to-hard time lags are detected in this object
for the first time. Cross-spectral results are consistent with those for other
accreting black hole systems. The results are discussed in the context of
several variability models, including those based on inwardly-propagating
viscosity variations in the accretion disk.Comment: Accepted for publication in The Astrophysical Journal. 18 pages, 9
figures. Uses emulateapj5.st
Superscaling predictions for neutrino-induced charged-current charged pion production at MiniBooNE
Superscaling approximation (SuSA) predictions to neutrino-induced
charged-current charged pion production in the \Delta-resonance region are
explored under MiniBooNE experimental conditions. The results obtained within
SuSA for the flux-averaged double-differential cross sections of the \pi+
production for the \nu_\mu+CH_2 reaction as a function of the muon kinetic
energy and of the scattering angle, the cross sections averaged over the angle,
the total cross section for the \pi+ production, as well as CC1\pi+ to CCQE
cross section ratio are compared with the corresponding MiniBooNE experimental
data. The SuSA predictions are in good agreement with data on neutrino flux
average cross-sections, but a somewhat different dependence on the neutrino
energy is predicted than the one resulting from the experimental analysis.Comment: 15 pages, 6 figures, accepted for publication in Physics Letters
Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured
Mergers of galaxies are thought to cause significant gas inflows to the inner
parsecs, which can activate rapid accretion onto supermassive black holes
(SMBHs), giving rise to Active Galactic Nuclei (AGN). During a significant
fraction of this process, SMBHs are predicted to be enshrouded by gas and dust.
Studying 52 galactic nuclei in infrared-selected local Luminous and
Ultra-luminous infrared galaxies in different merger stages in the hard X-ray
band, where radiation is less affected by absorption, we find that the amount
of material around SMBHs increases during the last phases of the merger. We
find that the fraction of Compton-thick (CT, ) AGN in late merger galaxies is higher
() than in local hard X-ray selected AGN
(), and that obscuration reaches its maximum when the
nuclei of the two merging galaxies are at a projected distance of
kiloparsecs (). We also
find that all AGN of our sample in late merger galaxies have , which implies that the obscuring material covers
of the X-ray source. These observations show that the material
is most effectively funnelled from the galactic scale to the inner tens of
parsecs during the late stages of galaxy mergers, and that the close
environment of SMBHs in advanced mergers is richer in gas and dust with respect
to that of SMBHs in isolated galaxies, and cannot be explained by the classical
AGN unification model in which the torus is responsible for the obscuration.Comment: Final version matching the article published in MNRAS - 30 pages, 16
figure
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