89,526 research outputs found
Information Flow in an R and D Laboratory
Statistical analysis of hypotheses concerning roles of technological gatekeeper and primary groups in flow of information in small research and development laborator
Large Magnetic Fields and Motions of OH Masers in W75 N
We report on a second epoch of VLBA observations of the 1665 and 1667 MHz OH
masers in the massive star-forming region W75 N. We find evidence to confirm
the existence of very strong (~40 mG) magnetic fields near source VLA 2. The
masers near VLA 2 are dynamically distinct and include a very bright spot
apparently moving at 50 km/s relative to those around VLA 1. This fast-moving
spot may be an example of a rare class of OH masers seen in outflows in
star-forming regions. Due to the variability of these masers and the rapidity
of their motions, tracking these motions will require multiple observations
over a significantly shorter time baseline than obtained here. Proper motions
of the masers near VLA 1 are more suggestive of streaming along magnetized
shocks rather than Keplerian rotation in a disk. The motions of the easternmost
cluster of masers in W75 N (B) may be tracing slow expansion around an unseen
exciting source.Comment: 7 pages including 4 figures (2 color) & 3 tables, to appear in Ap
Many-body theory of excitation dynamics in an ultracold Rydberg gas
We develop a theoretical approach for the dynamics of Rydberg excitations in
ultracold gases, with a realistically large number of atoms. We rely on the
reduction of the single-atom Bloch equations to rate equations, which is
possible under various experimentally relevant conditions. Here, we explicitly
refer to a two-step excitation-scheme. We discuss the conditions under which
our approach is valid by comparing the results with the solution of the exact
quantum master equation for two interacting atoms. Concerning the emergence of
an excitation blockade in a Rydberg gas, our results are in qualitative
agreement with experiment. Possible sources of quantitative discrepancy are
carefully examined. Based on the two-step excitation scheme, we predict the
occurrence of an antiblockade effect and propose possible ways to detect this
excitation enhancement experimentally in an optical lattice as well as in the
gas phase.Comment: 12 pages, 8 figure
Interactions Between Rydberg-Dressed Atoms
We examine interactions between atoms continuously and coherently driven
between the ground state and a Rydberg state, producing "Rydberg-dressed
atoms." Because of the large dipolar coupling between two Rydberg atoms, a
small admixture of Rydberg character into a ground state can produce an atom
with a dipole moment of a few Debye, the appropriate size to observe
interesting dipolar physics effects in cold atom systems. We have calculated
the interaction energies for atoms that interact via the dipole-dipole
interaction and find that due to blockade effects, the R-dependent two-atom
interaction terms are limited in size, and can be R-independent up until the
dipolar energy is equal to the detuning. This produces R-dependent interactions
different from the expected 1/R^3 dipolar form, which have no direct analogy in
condensed matter physics, and could lead to new quantum phases in trapped
Rydberg systems.Comment: 5 pages, 7 figures; Accepted to Phys. Rev. A, 18 Aug. 201
Model Independent Tests of Skyrmions and Their Holographic Cousins
We describe a new exact relation for large QCD for the long-distance
behavior of baryon form factors in the chiral limit. This model-independent
relation is used to test the consistency of the structure of several baryon
models. All 4D semiclassical chiral soliton models satisfy the relation, as
does the Pomarol-Wulzer holographic model of baryons as 5D Skyrmions. However,
remarkably, we find that the holographic model treating baryons as instantons
in the Sakai-Sugimoto model does not satisfy the relation.Comment: v2. Added references, corrected typo
One-year transitional programme increases knowledge to level sufficient for entry into the fourth year of the medical curriculum
BACKGROUND: To cope with a lack of doctors and in anticipation of the Bachelor-Master structure for Medicine, several Dutch universities offer graduate entry programmes for students with degrees in areas related to Medicine. The graduate entry programme is a four-year programme: after a transition period of one year students enroll in the fourth year of the regular six-year training programme. AIM: The research questions in this study were (1) whether and when graduate entry students' knowledge reached a level comparable to that of regular medical students and (2) whether there were differences in knowledge levels between graduate entry students with a university or HBO (college) degree. METHODS: The progress test results of ninety graduate entry students who were enrolled in the transitional programme between 2002 and 2004 were compared to those of regular third-year students. RESULTS: Initially, graduate entry students scored significantly lower on the progress tests, but differences disappeared within a year. No differences were found between graduate entry students with a university or HBO degree. CONCLUSIONS: The results of this study indicate that the increase in knowledge after a one-year transitional period is sufficient to enroll students with related degrees in the fourth year of the regular medical training programme
On The Importance Of The Interclump Medium For Superionization: O VI Formation In The Wind Of Zeta Puppis
We have studied superionization and X-ray line formation in the spectra of zeta Pup using our new stellar atmosphere code (XCMFGEN) that can be used to simultaneously analyze optical, UV, and X-ray observations. Here, we present results on the formation of the O VI lambda lambda 1032, 1038 doublet. Our simulations, supported by simple theoretical calculations, show that clumped wind models that assume void in the interclump space cannot reproduce the observed O vi profiles. However, enough O vi can be produced if the voids are filled by a low-density gas. The recombination of O vi is very efficient in the dense material, but in the tenuous interclump region an observable amount of O vi can be maintained. We also find that different UV resonance lines are sensitive to different density regimes in z Pup: C IV is almost exclusively formed within the densest regions, while the majority of O vi resides between clumps. N v is an intermediate case, with contributions from both the tenuous gas and clumps
Measurement of the ac Stark shift with a guided matter-wave interferometer
We demonstrate the effectiveness of a guided-wave Bose-Einstein condensate
interferometer for practical measurements. Taking advantage of the large arm
separations obtainable in our interferometer, the energy levels of the 87Rb
atoms in one arm of the interferometer are shifted by a calibrated laser beam.
The resulting phase shifts are used to determine the ac polarizability at a
range of frequencies near and at the atomic resonance. The measured values are
in good agreement with theoretical expectations. However, we observe a
broadening of the transition near the resonance, an indication of collective
light scattering effects. This nonlinearity may prove useful for the production
and control of squeezed quantum states.Comment: 5 pages, three figure
High-precision Measurements of Ionospheric TEC Gradients with the Very Large Array VHF System
We have used a relatively long, contiguous VHF observation of a bright cosmic
radio source (Cygnus A) with the Very Large Array (VLA) to demonstrate the
capability of this instrument to study the ionosphere. This interferometer, and
others like it, can observe ionospheric total electron content (TEC)
fluctuations on a much wider range of scales than is possible with many other
instruments. We have shown that with a bright source, the VLA can measure
differential TEC values between pairs of antennas (delta-TEC) with an precision
of 0.0003 TECU. Here, we detail the data reduction and processing techniques
used to achieve this level of precision. In addition, we demonstrate techniques
for exploiting these high-precision delta-TEC measurements to compute the TEC
gradient observed by the array as well as small-scale fluctuations within the
TEC gradient surface. A companion paper details specialized spectral analysis
techniques used to characterize the properties of wave-like fluctuations within
this data.Comment: accepted for publication in Radio Scienc
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