782 research outputs found
Reliability History and Improvements to the ANL 50 MEV H- Accelerator
The H- Accelerator consists of a 750 keV Cockcroft Walton preaccelerator and
an Alvarez type 50 MeV linac. The accelerator has been in operation since 1961.
Since 1981, it has been used as the injector for the Intense Pulsed Neutron
Source (IPNS), a national user facility for neutron scattering. The linac
delivers about 3.5x1012 H- ions per pulse, 30 times per second (30 Hz), for
multi-turn injection to a 450 MeV Rapid Cycling Synchrotron (RCS). IPNS
presently operates about 4,000 hours per year, and operating when scheduled is
critical to meeting the needs of the user community. For many years the IPNS
injector/RCS has achieved an average reliability of 95%, helped in large part
by the preaccelerator/linac which has averaged nearly 99%. To maintain and
improve system reliability, records need to show what each subsystem
contributes to the total down time. The history of source and linac subsystem
reliability, and improvements that have been made to improve reliability, will
be described. Plans to maintain or enhance this reliability for at least
another ten years of operation, will also be discussed.Comment: 3 pages, 1 figur
Nickel hydrogen low Earth orbit test program update and status
The current status of nickel-hydrogen (NiH2) testing ongong at NWSC, Crane In, and The Aerospace Corporation, El Segundo, Ca are described. The objective of this testing is to develop a database for NiH2 battery use in Low Earth Orbit (LEO) and support applications in Medium Altitude Orbit (MAO). Individual pressure vessel-type cells are being tested. A minimum of 200 cells (3.5 in diameter and 4.5 in diameter) are included in the test, from four U.S. vendors. As of this date (Nov. 18, 1986) approximately 60 cells have completed preliminary testing (acceptance, characterization, and environmental testing) and have gone into life cycling
X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
AGN are known to have complex X-ray spectra that depend on both the
properties of the accreting SMBH (e.g. mass, accretion rate) and the
distribution of obscuring material in its vicinity ("torus"). Often however,
simple and even unphysical models are adopted to represent the X-ray spectra of
AGN. In the case of blank field surveys in particular, this should have an
impact on e.g. the determination of the AGN luminosity function, the inferred
accretion history of the Universe and also on our understanding of the relation
between AGN and their host galaxies. We develop a Bayesian framework for model
comparison and parameter estimation of X-ray spectra. We take into account
uncertainties associated with X-ray data and photometric redshifts. We also
demonstrate how Bayesian model comparison can be used to select among ten
different physically motivated X-ray spectral models the one that provides a
better representation of the observations. Despite the use of low-count
spectra, our methodology is able to draw strong inferences on the geometry of
the torus. For a sample of 350 AGN in the 4 Ms Chandra Deep Field South field,
our analysis identifies four components needed to represent the diversity of
the observed X-ray spectra: (abridged). Simpler models are ruled out with
decisive evidence in favour of a geometrically extended structure with
significant Compton scattering. Regarding the geometry of the obscurer, there
is strong evidence against both a completely closed or entirely open toroidal
geometry, in favour of an intermediate case. The additional Compton reflection
required by data over that predicted by toroidal geometry models, may be a sign
of a density gradient in the torus or reflection off the accretion disk.
Finally, we release a catalogue with estimated parameters such as the accretion
luminosity in the 2-10 keV band and the column density, , of the
obscurer.Comment: 28 pages, 18 figures, catalogue available from
https://www.mpe.mpg.de/~jbuchner/agn_torus/analysis/cdfs4Ms_cat/, software
available from https://github.com/JohannesBuchner/BX
Bose-Einstein condensate collapse: a comparison between theory and experiment
We solve the Gross-Pitaevskii equation numerically for the collapse induced
by a switch from positive to negative scattering lengths. We compare our
results with experiments performed at JILA with Bose-Einstein condensates of
Rb-85, in which the scattering length was controlled using a Feshbach
resonance. Building on previous theoretical work we identify quantitative
differences between the predictions of mean-field theory and the results of the
experiments. Besides the previously reported difference between the predicted
and observed critical atom number for collapse, we also find that the predicted
collapse times systematically exceed those observed experimentally. Quantum
field effects, such as fragmentation, that might account for these
discrepancies are discussed.Comment: 4 pages, 2 figure
Tree-body loss of of trapped ultracold Rb atoms due to a Feshbach resonance
The loss of ultracold trapped atoms in the vicinity of a Feshbach resonance
is treated as a two-stage reaction, using the Breit-Wigner theory. The first
stage is the formation of a resonant diatomic molecule, and the second one is
its deactivation by inelastic collisions with other atoms. This model is
applied to the analysis of recent experiments on Rb, leading to an
estimated value of cms for the deactivation rate
coefficient.Comment: LaTeX, 4 pages with 1 figures, uses REVTeX4, uses improved
experimental dat
Stability of fermionic Feshbach molecules in a Bose-Fermi mixture
In the wake of successful experiments in Fermi condensates, experimental
attention is broadening to study resonant interactions in degenerate Bose-Fermi
mixtures. Here we consider the properties and stability of the fermionic
molecules that can be created in such a mixture near a Feshbach resonance (FR).
To do this, we consider the two-body scattering matrix in the many-body
environment, and assess its complex poles. The stability properties of these
molecules strongly depend on their centre-of-mass motion, because they must
satisfy Fermi statistics. At low centre-of-mass momenta the molecules are more
stable than in the absence of the environment (due to Pauli-blocking effects),
while at high centre-of-mass momenta nontrivial many body effects render them
somewhat less stable
Unveiling a Population of X-ray Non-Detected AGN
We define a sample of 27 radio-excess AGN in the Chandra Deep Field North by
selecting galaxies that do not obey the radio/infrared correlation for
radio-quiet AGN and star-forming galaxies. Approximately 60% of these
radio-excess AGN are X-ray undetected in the 2 Ms Chandra catalog, even at
exposures of > 1 Ms; 25% lack even 2-sigma X-ray detections. The absorbing
columns to the faint X-ray-detected objects are 10^22 cm^-2 < N_H < 10^24
cm^-2, i.e., they are obscured but unlikely to be Compton thick. Using a local
sample of radio-selected AGN, we show that a low ratio of X-ray to radio
emission, as seen in the X-ray weakly- and non-detected samples, is correlated
with the viewing angle of the central engine, and therefore with obscuration.
Our technique can explore the proportion of obscured AGN in the distant
Universe; the results reported here for radio-excess objects are consistent
with but at the low end of the overall theoretical predictions for
Compton-thick objects.Comment: Accepted for publication in the Astrophysical Journal, 15 pages, 10
figures, 4 table
A microscopic quantum dynamics approach to the dilute condensed Bose gas
We derive quantum evolution equations for the dynamics of dilute condensed
Bose gases. The approach contains, at different orders of approximation, for
cases close to equilibrium, the Gross Pitaevskii equation and the first order
Hartree Fock Bogoliubov theory. The proposed approach is also suited for the
description of the dynamics of condensed gases which are far away from
equilibrium. As an example the scattering of two Bose condensates is discussed.Comment: 8 pages, submitted to Phys. Rev.
Morphologies of Radio, X-Ray, and Mid-Infrared Selected AGN
We investigate the optical morphologies of candidate active galaxies
identified at radio, X-ray, and mid-infrared wavelengths. We use the Advanced
Camera for Surveys General Catalog (ACS-GC) to identify 372, 1360, and 1238 AGN
host galaxies from the VLA, XMM-Newton and Spitzer Space Telescope observations
of the COSMOS field, respectively. We investigate both quantitative (GALFIT)
and qualitative (visual) morphologies of these AGN host galaxies, split by
brightness in their selection band. We find that the radio-selected AGN are
most distinct, with a very low incidence of having unresolved optical
morphologies and a high incidence of being hosted by early-type galaxies. In
comparison to X-ray selected AGN, mid-IR selected AGN have a slightly higher
incidence of being hosted by disk galaxies. These morphological results conform
with the results of Hickox et al. 2009 who studied the colors and large-scale
clustering of AGN, and found a general association of radio-selected AGN with
``red sequence'' galaxies, mid-IR selected AGN with ``blue cloud'' galaxies,
and X-ray selected AGN straddling these samples in the ``green valley.'' In the
general scenario where AGN activity marks and regulates the transition from
late-type disk galaxies into massive elliptical galaxies, this work suggests
that the earlier stages are most evident as mid-IR selected AGNs. Mid-IR
emission is less susceptible to absorption than the relatively soft X-rays
probed by XMM-Newton, which are seen at later stages in the transition.
Radio-selected AGN are then typically associated with minor bursts of activity
in the most massive galaxies.Comment: 28 page
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