2,598 research outputs found
Analysis of the instantaneous Bethe-Salpeter equation for -bound-states
We investigate the structure of the instantaneous Bethe-Salpeter equation for
-bound states in the general case of unequal quark masses and
develop a numerical scheme for the calculation of mass spectra and
Bethe-Salpeter amplitudes. In order to appreciate the merits of the various
competing models beyond the reproduction of the mass spectra we present
explicit formulas to calculate electroweak decays. The results for an explicit
quark model will be compared to experimental data in a subsequent paperComment: 11 pages, RevTeX, TK-93-1
Generalized parton distributions and double distributions for q q-bar pions
We consider two simple covariant models for pions (one with scalar and the
other with spin-1/2 constituents). Pion generalized parton distributions are
derived by integration over the light-cone energy. The model distributions are
consistent with all known properties of generalized parton distributions,
including positivity. We also construct the corresponding double distributions
by appealing to Lorentz invariance. These ostensibly constructed double
distributions lead to different generalized parton distributions that need not
respect the positivity constraints. This inconsistency arises from the
ambiguity inherent in defining double distributions in a one-component
formalism (even in the absence of the Polyakov-Weiss term). We demonstrate that
the correct model double distributions can be calculated from non-diagonal
matrix elements of twist-two operators.Comment: 10 pages, 7 figures, RevTex4, reference added, typos correcte
A Bethe-Salpeter model for light mesons: spectra and decays
The spectra and electroweak decay properties of light mesons are analyzed
within the framework of the instantaneous Bethe-Salpeter equation. The
interaction kernel comprises alternative spin-structures for a parameterization
of confinement and a residual quark-antiquark interaction based on instanton
effects. It is shown that only with a vector confinement the parameters can be
chosen such as to yield an excellent description of the light pseudoscalar and
vector mesons including weak and two photon decays. However it is found that it
is not possible to reconcile this with the Regge behavior of higher lying meson
states with the same parameter set.Comment: 12 pages, RevTeX, TK-93-1
KamLAND Bounds on Solar Antineutrinos and neutrino transition magnetic moments
We investigate the possibility of detecting solar electron antineutrinos with
the KamLAND experiment. These electron antineutrinos are predicted by
spin-flavor oscillations at a significant rate even if this mechanism is not
the leading solution to the SNP. KamLAND is sensitive to antineutrinos
originated from solar B neutrinos. From KamLAND negative results after
145 days of data taking, we obtain model independent limits on the total flux
of solar electron antineutrinos $\Phi({}^8 B)< 1.1-3.5\times 10^4 cm^{-2}\
s^{-1}P<0.15%\mu B< 2.3\times 10^{-21}(\Delta m^2, \tan^2\theta)\mu\lsim 3.9\times 10^{-12} \mu_BB= 50\mu\lsim 9.0\times 10^{-13} \mu_BB= 200\mu\lsim 2.0\times 10^{-13} \mu_BB= 1000$ kG at the same
statistical significance.Comment: 13 pages, 2 figure
Cystic Fibrosis Foundation and European Cystic Fibrosis Society Survey of cystic fibrosis mental health care delivery
Background: Psychological morbidity in individuals with cystic fibrosis (CF) and their caregivers is common. The Cystic Fibrosis Foundation (CFF) and European Cystic Fibrosis Society (ECFS) Guidelines Committee on Mental Health sought the views of CF health care professionals concerning mental health care delivery.
Methods: An online survey which focused on the current provision and barriers to mental health care was distributed to CF health care professionals.
Results: Of the 1454 respondents, many did not have a colleague trained in mental health issues and 20% had no one on their team whose primary role was focused on assessing or treating these issues. Insufficient resources and a lack of competency were reported in relation to mental health referrals. Seventy-three percent of respondents had no experience with mental health screening. Of those who did, they utilized 48 different, validated scales.
Conclusions: These data have informed the decision-making, dissemination and implementation strategies of the Mental Health Guidelines Committee sponsored by the CFF and ECFS
Status of Grey Leaf Spot Disease In Kenyan Maize Production Ecosystems
Grey leaf spot disease (GLS), Cercospora zeae-maydis, which has
previously been attributed to diverse pathogen species in other
countries, has become a serious biotic constraint to production of
maize ( Zea mays L.) in Kenya. It is necessary to determine the
distribution and aetiology of the disease across all the maize
production agro-ecologies in order to inform the development of
appropriate management strategies against the disease. Samples were
collected from maize growing areas in Kenya with GLS symptoms on maize
crops and other plants. On the basis of cultural and morphological
examinations, and restricted fragment length polymorphism and
taxon-specific PCR analyses, Cercospora zeae-maydis group II and C.
sorghi var. maydis were identified from typical GLS lesions on maize,
with the former being predominant (>96% of the cases) and
distributed throughout the country. The latter exhibited minor
incidence (<4%) in western Kenya. Nucleotide sequence analyses
further provided evidence that C. zeae-maydis group II and C. sorghi
var. maydis were distinct fungi.La maladie de t\ue2che grise de la feuille (GLS), Cercospora
zeae-maydis, attribu\ue9e aux esp\ue8ces de pathogens diverses dans
d'autres pays, est devenue une s\ue9rieuse contrainte biotique \ue0
la production de ma\uefs ( Zea mays L.) au Kenya. Il est
n\ue9cessaire de d\ue9terminer la distribution et l'\ue9tiologie
de la maladie \ue0 travers toutes les r\ue9gions
agro-\ue9cologques productrices de ma\uefs pour mieux
d\ue9velopper des strat\ue9gies appropri\ue9es de gestion contre
la maladie. Des \ue9chantillons \ue9taient recueillis dans des
r\ue9gions producteurs du ma\uefs au Kenya tenant compte de la
pr\ue9sence des sympt\uf4mes GLS sur les ma\uefs et autres
cultures. Sur base des examens culturales et morphologiques ainsi que
du polymorphisme de la longueur du fragment isol\ue9 et les analyses
PCR du taxon sp\ue9cifique, Cercospora zeae-maydis le groupe II de
Cercospora zeae-maydis et C. sorghi var. maydis \ue9taient
identifi\ue9s par des l\ue9sions typiques de GLS sur le ma\uefs,
ce dernier \ue9tant le plus pr\ue9dominant (> 96 % de tous les
cas) et distribu\ue9 \ue0 travers tout le pays avec une incidence
mineur de 4 % dans l'ouest du Kenya. L'analyse de s\ue9quences de
nucl\ue9otides avait par la suite montr\ue9 avec evidence que le C.
zeae-maydis group II et C. sorghi var. maydis \ue9taient de
champignons distincts
Mathematical Model of the Oxidation of a Uranium Carbide Fuel Pellet Including an Adherent Product Layer
Uranium carbide is a candidate fuel for Generation IV nuclear reactors. However, like any candidate fuel, a reprocessing route should be established before implementation. One proposed method involves a pre-oxidation step, where the carbide fuel is oxidised to an oxide and then reprocessed as normal. A mathematical model has been developed to simulate such an oxidation using finite difference approximations of the heat and mass transfer processes occurring. Available literature was consulted to provide coefficients for the reaction rates and importantly the diffusion of oxygen through the adherent oxide layer that forms on the carbide: the rate limiting step. The transient temperature, oxygen and carbon monoxide distributions through the system are modelled in order to predict oxidation completion times and the temperatures reached. It was found that for a spherical pellet of radius 0.935cm, the oxidation can take between 1 h to 19 h depending on the oxidation conditions and reach temperatures of up to 1556°C. A robust model results that offers increased understanding of a process crucial to the sustainable use of carbide fuels in energy generation
Star and cluster formation in extreme environments
Current empirical evidence on the star-formation processes in the extreme,
high-pressure environments induced by galaxy encounters (mostly based on
high-resolution Hubble Space Telescope observations) strongly suggests that
star CLUSTER formation is an important and perhaps even the dominant mode of
star formation in such starburst events. The sizes, luminosities, and mass
estimates of the young massive star clusters (YMCs) are entirely consistent
with what is expected for young Milky Way-type globular clusters (GCs). Recent
evidence lends support to the scenario that GCs, which were once thought to be
the oldest building blocks of galaxies, are still forming today. Here, I
present a novel empirical approach to assess the shape of the
initial-to-current YMC mass functions, and hence their possible survival
chances for a Hubble time.Comment: 6 pages, LaTeX with Kluwer style files included; to appear in:
"Starbursts - from 30 Doradus to Lyman break galaxies" (Cambridge UK,
September 2004; talk summary), Astrophysics & Space Science Library, eds. de
Grijs R., Gonzalez Delgado R.M., Kluwer: Dordrech
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