2,226 research outputs found
Quantum dynamical response of ultracold few boson ensembles in finite optical lattices to multiple interaction quenches
The correlated non-equilibrium quantum dynamics following a multiple
interaction quench protocol for few-bosonic ensembles confined in finite
optical lattices is investigated. The quenches give rise to an interwell
tunneling and excite the cradle and a breathing mode. Several tunneling
pathways open during the time interval of increased interactions, while only a
few occur when the system is quenched back to its original interaction
strength. The cradle mode, however, persists during and in between the
quenches, while the breathing mode possesses dinstinct frequencies. The
occupation of excited bands is explored in detail revealing a monotonic
behavior with increasing quench amplitude and a non-linear dependence on the
duration of the application of the quenched interaction strength. Finally, a
periodic population transfer between momenta for quenches of increasing
interaction is observed, with a power-law frequency dependence on the quench
amplitude. Our results open the possibility to dynamically manipulate various
excited modes of the bosonic system.Comment: 13 pages, 9 figure
Photochemical Electrocyclic Ring Closure and Leaving Group Expulsion from N-(9-oxothioxanthenyl)Benzothiophene Carboxamides
N-(9-Oxothioxanthenyl)benzothiophene carboxamides bearing leaving groups (LG− = Cl−, PhS−, HS−, PhCH2S−) at the C-3 position of the benzothiophene ring system photochemically cyclize with nearly quantitative release of the leaving group, LG−. The LG− photoexpulsions can be conducted with 390 nm light or with a sunlamp. Solubility in 75% aqueous CH3CN is achieved by introducing a carboxylate group at the C-6 position of the benzothiophene ring. The carboxylate and methyl ester derivatives regiospecifically cyclize at the more hindered C-1 position of the thioxanthone ring. Otherwise, the photocyclization favors the C-3 position of the thioxanthone. Quantum yields for reaction are 0.01–0.04, depending on LG− basicity. Electronic structure calculations for the triplet excited state show that excitation transfer occurs from the thioxanthone to the benzothiophene ring. Subsequent cyclization in the triplet excited state is energetically favourable and initially generates the triplet excited state of the zwitterionic species. Expulsion of LG− is thought to occur once this species converts to the closed shell ground state
Planes of satellite galaxies and the cosmic web
Recent observational studies have demonstrated that the majority of satellite
galaxies tend to orbit their hosts on highly flattened, vast, possibly
co-rotating planes. Two nearly parallel planes of satellites have been
confirmed around the M31 galaxy and around the Centaurus A galaxy, while the
Milky Way also sports a plane of satellites. It has been argued that such an
alignment of satellites on vast planes is unexpected in the standard
({\Lambda}CDM) model of cosmology if not even in contradiction to its generic
predictions. Guided by {\Lambda}CDM numerical simulations, which suggest that
satellites are channeled towards hosts along the axis of the slowest collapse
as dictated by the ambient velocity shear tensor, we re-examine the planes of
local satellites systems within the framework of the local shear tensor derived
from the Cosmicflows-2 dataset. The analysis reveals that the Local Group and
Centaurus A reside in a filament stretched by the Virgo cluster and compressed
by the expansion of the Local Void. Four out of five thin planes of satellite
galaxies are indeed closely aligned with the axis of compression induced by the
Local Void. Being the less massive system, the moderate misalignment of the
Milky Way's satellite plane can likely be ascribed to its greater
susceptibility to tidal torques, as suggested by numerical simulations. The
alignment of satellite systems in the local universe with the ambient shear
field is thus in general agreement with predictions of the {\Lambda}CDM model.Comment: 9 pages, 3 figures, 3 tables. Accepted by MNRAS, 9 June 201
The influence of baryons on the mass distribution of dark matter halos
Using a set of high-resolution N-body/SPH cosmological simulations with
identical initial conditions but run with different numerical setups, we
investigate the influence of baryonic matter on the mass distribution of dark
halos when radiative cooling is NOT included. We compare the concentration
parameters of about 400 massive halos with virial mass from \Msun to
\Msun. We find that the concentration parameters for the
total mass and dark matter distributions in non radiative simulations are on
average larger by ~3% and 10% than those in a pure dark matter simulation. Our
results indicate that the total mass density profile is little affected by a
hot gas component in the simulations. After carefully excluding the effects of
resolutions and spurious two-body heating between dark matter and gas
particles, we conclude that the increase of the dark matter concentration
parameters is due to interactions between baryons and dark matter. We
demonstrate this with the aid of idealized simulations of two-body mergers. The
results of individual halos simulated with different mass resolutions show that
the gas profiles of densities, temperature and entropy are subjects of mass
resolution of SPH particles. In particular, we find that in the inner parts of
halos, as the SPH resolution increases the gas density becomes higher but both
the entropy and temperature decrease.Comment: 8 pages, 6 figures, 1 table, ApJ in press (v652n1); updated to match
with the being published versio
The alignment of galaxy spin with the shear field in observations
Tidal torque theory suggests that galaxies gain angular momentum in the
linear stage of structure formation. Such a theory predicts alignments between
the spin of haloes and tidal shear field. However, non-linear evolution and
angular momentum acquisition may alter this prediction significantly. In this
paper, we use a reconstruction of the cosmic shear field from observed peculiar
velocities combined with spin axes extracted from galaxies within () from 2MRS
catalog, to test whether or not galaxies appear aligned with principal axes of
shear field. Although linear reconstructions of the tidal field have looked at
similar issues, this is the first such study to examine galaxy alignments with
velocity-shear field. Ellipticals in the 2MRS sample, show a statistically
significant alignment with two of the principal axes of the shear field. In
general, elliptical galaxies have their short axis aligned with the axis of
greatest compression and perpendicular to the axis of slowest compression.
Spiral galaxies show no signal. Such an alignment is significantly strengthened
when considering only those galaxies that are used in velocity field
reconstruction. When examining such a subsample, a weak alignment with the axis
of greatest compression emerges for spiral galaxies as well. This result
indicates that although velocity field reconstructions still rely on fairly
noisy and sparse data, the underlying alignment with shear field is strong
enough to be visible even when small numbers of galaxies are considered -
especially if those galaxies are used as constraints in the reconstruction.Comment: 9 pages, 3 figures, accepted in MNRA
Engineering chromium related single photon emitters in single crystal diamond
Color centers in diamond as single photon emitters, are leading candidates
for future quantum devices due to their room temperature operation and
photostability. The recently discovered chromium related centers are
particularly attractive since they possess narrow bandwidth emission and a very
short lifetime. In this paper we investigate the fabrication methodologies to
engineer these centers in monolithic diamond. We show that the emitters can be
successfully fabricated by ion implantation of chromium in conjunction with
oxygen or sulfur. Furthermore, our results indicate that the background
nitrogen concentration is an important parameter, which governs the probability
of success to generate these centers.Comment: 14 pages, 5 figure
Galactic Archaeology with CoRoT and APOGEE: Creating mock observations from a chemodynamical model
In a companion paper, we have presented the combined
asteroseismic-spectroscopic dataset obtained from CoRoT lightcurves and APOGEE
infra-red spectra for 678 solar-like oscillating red giants in two fields of
the Galactic disc (CoRoGEE). We have measured chemical abundance patterns,
distances, and ages of these field stars which are spread over a large radial
range of the Milky Way's disc. Here we show how to simulate this dataset using
a chemodynamical Galaxy model. We also demonstrate how the observation
procedure influences the accuracy of our estimated ages.Comment: 5 pages, 6 figures. To appear in Astronomische Nachrichten, special
issue "Reconstruction the Milky Way's History: Spectroscopic surveys,
Asteroseismology and Chemo-dynamical models", Guest Editors C. Chiappini, J.
Montalb\'an, and M. Steffe
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