9,651 research outputs found
Non-equilibrium chemistry and dust formation in AGB stars as probed by SiO line emission
We have performed high spatial resolution observations of SiO line emission
for a sample of 11 AGB stars using the ATCA, VLA and SMA interferometers.
Detailed radiative transfer modelling suggests that there are steep chemical
gradients of SiO in their circumstellar envelopes. The emerging picture is one
where the radial SiO abundance distribution starts at an initial high
abundance, in the case of M-stars consistent with LTE chemistry, that
drastically decreases at a radius of ~1E15 cm. This is consistent with a
scenario where SiO freezes out onto dust grains. The region of the wind with
low abundance is much more extended, typically ~1E16 cm, and limited by
photodissociation. The surpisingly high SiO abundances found in carbon stars
requires non-equilibrium chemical processes.Comment: 2 pages, 1 figure. To be published in the proceedings of the
conference "Why Galaxies Care about AGB Stars", held in Vienna, August 7-11,
2006; F. Kerschbaum, C. Charbonnel, B. Wing eds, ASP Conf.Ser. in pres
Ground-state fidelity in one-dimensional gapless model
A general relation between quantum phase transitions and the second
derivative of the fidelity (or the "fidelity susceptibility") is proposed. The
validity and the limitation of the fidelity susceptibility in characterizing
quantum phase transitions is thus established. Moreover, based on the
bosonization method, general formulas of the fidelity and the fidelity
susceptibility are obtained for a class of one-dimensional gapless systems
known as the Tomonaga-Luttinger liquid. Applying these formulas to the
one-dimensional spin-1/2 model, we find that quantum phase transitions,
even of the Beresinskii-Kosterlitz-Thouless type, can be signaled by the
fidelity susceptibility.Comment: 4+ pages, no figure, published versio
High energy spin excitations in YBa_2 Cu_3 O_{6.5}
Inelastic neutron scattering has been used to obtain a comprehensive
description of the absolute dynamical spin susceptibility
of the underdoped superconducting cuprate YBa_2 Cu_3 O_{6.5} ()
over a wide range of energies and temperatures ( and ). Spin excitations of two different
symmetries (even and odd under exchange of two adjacent CuO_2 layers) are
observed which, surprisingly, are characterized by different temperature
dependences. The excitations show dispersive behavior at high energies.Comment: 15 pages, 5 figure
Exchange-Only Dynamical Decoupling in the 3-Qubit Decoherence Free Subsystem
The Uhrig dynamical decoupling sequence achieves high-order decoupling of a
single system qubit from its dephasing bath through the use of bang-bang Pauli
pulses at appropriately timed intervals. High-order decoupling of single and
multiple qubit systems from baths causing both dephasing and relaxation can
also be achieved through the nested application of Uhrig sequences, again using
single-qubit Pauli pulses. For the 3-qubit decoherence free subsystem (DFS) and
related subsystem encodings, Pauli pulses are not naturally available
operations; instead, exchange interactions provide all required encoded
operations. Here we demonstrate that exchange interactions alone can achieve
high-order decoupling against general noise in the 3-qubit DFS. We present
decoupling sequences for a 3-qubit DFS coupled to classical and quantum baths
and evaluate the performance of the sequences through numerical simulations
A four month prospective descriptive exploratory study of patients receiving antibiotics in one Emergency Department
Background: Any infection can potentially develop into sepsis. Many patients present to the Emergency Department (ED) with infection and go on to require antibiotics. However, the timeliness of antibiotics can make a difference to patient survival and reduce the risk of infection developing into sepsis and or septic shock. Methods: Our study was a 4. month prospective descriptive exploratory pilot study. Results: Of all adult (n = 18,807) presentations 3339 (18%) patients had a primary diagnosis related to infection. The study collected data on 104 (3%) patients who were administered antibiotics. One hundred (95%) patients who received antibiotics were admitted to hospital. Triage code did not influence time to antibiotic (p = .352). Eighty-five (81%) patients waited longer than 1. h for their first antibiotic with the shortest administration time 19. min (mean 233. min, SD 247) and the maximum wait for antibiotics was 1481. min. For sepsis or septic shock patients (n = 8) the average time to antibiotics was 411. min (SD. = 455. min). Conclusion: The study provides a detailed analysis of ED patients receiving antibiotics. Further research is needed to identify strategies to improve the timely delivery of antibiotics for patients with infections. © 2012 Elsevier Ltd
Supersymmetric Leptogenesis
We study leptogenesis in the supersymmetric standard model plus the seesaw.
We identify important qualitative differences that characterize supersymmetric
leptogenesis with respect to the non-supersymmetric case. The lepton number
asymmetries in fermions and scalars do not equilibrate, and are related via a
non-vanishing gaugino chemical potential. Due to the presence of new anomalous
symmetries, electroweak sphalerons couple to winos and higgsinos, and QCD
sphalerons couple to gluinos, thus modifying the corresponding chemical
equilibrium conditions. A new constraint on particles chemical potentials
corresponding to an exactly conserved -charge, that also involves the number
density asymmetry of the heavy sneutrinos, appears. These new ingredients
determine the matrices that mix up the density asymmetries of the
lepton flavours and of the heavy sneutrinos. We explain why in all temperature
ranges the particle thermodynamic system is characterized by the same number of
independent quantities. Numerical differences with respect to usual treatment
remain at the level.Comment: 30 pages, 2 figures. Typos corrected, one reference added. Version
published in JCA
Quantum Impurities and the Neutron Resonance Peak in : Ni versus Zn
The influence of magnetic (S=1) and nonmagnetic (S=0) impurities on the spin
dynamics of an optimally doped high temperature superconductor is compared in
two samples with almost identical superconducting transition temperatures:
YBa(CuNi)O (T=80 K) and
YBa(CuZn)O (T=78 K). In the Ni-substituted
system, the magnetic resonance peak (which is observed at E40 meV in
the pure system) shifts to lower energy with a preserved E/T ratio
while the shift is much smaller upon Zn substitution. By contrast Zn, but not
Ni, restores significant spin fluctuations around 40 meV in the normal state.
These observations are discussed in the light of models proposed for the
magnetic resonance peak.Comment: 3 figures, submitted to PR
World-wide epidemiology of HBeAg-negative chronic hepatitis B and associated precore and core promoter variants
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/72281/1/j.1365-2893.2002.00304.x.pd
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