2,142 research outputs found
Criticality in multicomponent spherical models : results and cautions
To enable the study of criticality in multicomponent fluids, the standard
spherical model is generalized to describe an \ns-species hard core lattice
gas. On introducing \ns spherical constraints, the free energy may be
expressed generally in terms of an \ns\times\ns matrix describing the species
interactions. For binary systems, thermodynamic properties have simple
expressions, while all the pair correlation functions are combinations of just
two eigenmodes. When only hard-core and short-range overall attractive
interactions are present, a choice of variables relates the behavior to that of
one-component systems. Criticality occurs on a locus terminating a coexistence
surface; however, except at some special points, an unexpected
``demagnetization effect'' suppresses the normal divergence of susceptibilities
at criticality and distorts two-phase coexistence. This effect, unphysical for
fluids, arises from a general lack of symmetry and from the vectorial and
multicomponent character of the spherical model. Its origin can be understood
via a mean-field treatment of an XY spin system below criticality.Comment: 4 figure
Coordination sécurité pour la phase génie civil du projet LHC
Partant des constatations que le risque d'accident est deux fois plus important dans le BTP que dans les autres branches d'activité et que 60% des accidents dans le BTP proviennent de choix effectués avant travaux, une directive européenne a été élaborée et a donné naissance à des textes de loi français. La principale mesure résultant de ces textes est la désignation, par le maître d'ouvrage d'un coordonnateur sécurité. Ce coordonnateur est chargé, entre autres, de prévenir les risques de coactivités des entreprises. Il intervient dès la phase de conception en vue d'analyser et de prévenir les risques sur le chantier et dans les interventions ultérieures. Les textes de loi décrivent également les notions de déclarations préalables, aux autorités compétentes, les plans de sécurité rédigés par le coordonnateur et les entreprises, ainsi que le dossier rassemblant les éléments utiles en matière de sécurité et de santé pour d'éventuels travaux ultérieurs. Toutes ces dispositions sont mises en application par le groupe Génie civil du CERN pour la réalisation des ouvrages du projet LHC
Stellar Populations in the Outskirts of the Small Magellanic Cloud: No Outer Edge Yet
We report the detection of intermediate-age and old stars belonging to the
SMC at 6.5 kpc from the SMC center in the southern direction. We show, from the
analysis of three high quality 34\arcmin 33\arcmin CMDs, that the age
composition of the stellar population is similar at galactocentric distances of
4.7 kpc, 5.6 kpc, and 6.5 kpc. The surface
brightness profile of the SMC follows an exponential law, with no evidence of
truncation, all the way out to 6.5 kpc. These results, taken together, suggest
that the SMC `disk' population is dominating over a possible old Milky Way-like
stellar halo, and that the SMC may be significantly larger than previously
thought.Comment: Accepted for publication in ApJ Letters. High resolution figures are
available at ftp://ftp.iac.es/out/noe
Stellar populations in the surrounding field of the LMC clusters NGC 2154 and NGC 1898
In this paper we present a study and comparison of the star formation rates
(SFR) in the fields around NGC 1898 and NGC 2154, two intermediate-age star
clusters located in very different regions of the Large Magellanic Cloud. We
also present a photometric study of NGC 1898, and of seven minor clusters which
happen to fall in the field of NGC 1898, for which basic parameters were so far
unknown. We do not focus on NGC 2154, because this cluster was already
investigated in Baume et al. 2007, using the same theoretical tools. The ages
of the clusters were derived by means of the isochrone fitting method on their
color-magnitude diagrams. Two distinct populations of clusters were
found: one cluster (NGC 2154) has a mean age of 1.7 Gyr, with indication of
extended star formation over roughly a 1 Gyr period, while all the others have
ages between 100 and 200 Myr. The SFRs of the adjacent fields were inferred
using the downhill-simplex algorithm. Both SFRs show enhancements at 200, 400,
800 Myr, and at 1, 6, and 8 Gyr. These bursts in the SFR are probably the
result of dynamical interactions between the Magellanic Clouds (MCs), and of
the MCs with the Milky Way.Comment: 10 pages, 11 eps figures, in press in MNRAS. For a version including
references contact the author
The Challenges of Multimorbidity from the Patient Perspective
BACKGROUND
Although multiple co-occurring chronic illnesses within the same individual are increasingly common, few studies have examined the challenges of multimorbidity from the patient perspective.
OBJECTIVE
The aim of this study is to examine the self-management learning needs and willingness to see non-physician providers of patients with multimorbidity compared to patients with single chronic illnesses. DESIGN. This research is designed as a cross-sectional survey.
PARTICIPANTS
Based upon ICD-9 codes, patients from a single VHA healthcare system were stratified into multimorbidity clusters or groups with a single chronic illness from the corresponding cluster. Nonproportional sampling was used to randomly select 720 patients.
MEASUREMENTS
Demographic characteristics, functional status, number of contacts with healthcare providers, components of primary care, self-management learning needs, and willingness to see nonphysician providers.
RESULTS
Four hundred twenty-two patients returned surveys. A higher percentage of multimorbidity patients compared to single morbidity patients were "definitely" willing to learn all 22 self-management skills, of these only 2 were not significant. Compared to patients with single morbidity, a significantly higher percentage of patients with multimorbidity also reported that they were "definitely" willing to see 6 of 11 non-physician healthcare providers.
CONCLUSIONS
Self-management learning needs of multimorbidity patients are extensive, and their preferences are consistent with team-based primary care. Alternative methods of providing support and chronic illness care may be needed to meet the needs of these complex patients.US Department of Veterans Affairs (01-110, 02-197); Agency for Healthcare Research and Quality (K08 HS013008-02
Towards Earlier Identification: Physicians Assistants\u27 Perceptions of their Ability to Identify, Diagnose, and Refer Patients with Autism Spectrum Disorder.
Heavy fermion superconductivity and magnetic order in non-centrosymmetric
is a novel heavy fermion superconductor, crystallising in the
structure as a tetragonally distorted low symmetry variant of the
structure type. exhibits antiferromagnetic order at
K and enters into a heavy fermion superconducting state at
K. Large values of T/K and T refer to heavy quasiparticles forming Cooper pairs. Hitherto, is the first heavy fermion superconductor without a center of
symmetry.Comment: 4 pages, 4 figure
The Chemical Enrichment History of the Small Magellanic Cloud and Its Gradients
We present stellar metallicities derived from Ca II triplet spectroscopy in
over 350 red giant branch stars in 13 fields distributed in different positions
in the SMC, ranging from 1\arcdeg\@ to 4\arcdeg\@ from its center.
In the innermost fields the average metallicity is [Fe/H] . This value
decreases when we move away towards outermost regions. This is the first
detection of a metallicity gradient in this galaxy. We show that the
metallicity gradient is related to an age gradient, in the sense that more
metal-rich stars, which are also younger, are concentrated in the central
regions of the galaxy.Comment: 30 pages, 13 figures, accepted for publication in Astronomical
Journa
- …