Propagation of mesons in asymmetric nuclear matter in a density dependent coupling model

We study the propagation of the light mesons sigma, omega, rho, and a0(980) in dense hadronic matter in an extended derivative scalar coupling model. Within the scheme proposed it is possible to unambiguously define effective density-dependent couplings at the Lagrangian level. We first apply the model to study asymmetric nuclear matter with fixed isospin asymmetry, and then we pay particular attention to hypermatter in beta-equilibrium. The equation of state and the potential contribution to the symmetry coefficient arising from the mean field approximation are investigated.Comment: 17 pages, 15 PostScript figure

Landau parameters for isospin asymmetric nuclear matter based on a relativistic model of composite and finite extension nucleons

We study the properties of cold asymmetric nuclear matter at high density, applying the quark meson coupling model with excluded volume corrections in the framework of the Landau theory of relativistic Fermi liquids. We discuss the role of the finite spatial extension of composite baryons on dynamical and statistical properties such as the Landau parameters, the compressibility, and the symmetry energy. We have also calculated the low lying collective eigenfrequencies arising from the collisionless quasiparticle transport equation, considering both unstable and stable modes. An overall analysis of the excluded volume correlations on the collective properties is performed.Comment: 24 pages, 6 figure

Molecular methods for the identification of Aspergillus species

Invasive aspergillosis (IA) is a leading cause of morbidity and mortality in immunocompromised hosts. In some institutions, species of Aspergillus less susceptible to amphotericin B than Aspergillus fumigatus are becoming more common, making an accurate identification of species important. However, species identification has traditionally relied on macroscopic colony characteristics and microscopic morphology, which may require several days of culture. Additional sub-culturing on specialized media may be required to induce conidia formation; in some cases conidia may never form, confounding identification. Therefore, rapid, nucleic acid-based methods that identify species of Aspergillus independent of morphology are now being developed to augment or replace phenotypic identification methods. The most successful methods to date have employed polymerase chain reaction (PCR) amplification of target sequences within the ribosomal RNA gene complex, including the 28S ribosomal subunit (D1-D2 region) and the internal transcribed spacers 1 and 2 (ITS1 and ITS2 regions). We therefore developed a PCR-based assay to differentiate medically important species of Aspergillus from one another, and from other opportunistic moulds and yeasts, by employing universal, pan-fungal primers directed to conserved ribosomal genes and species-specific DNA probes directed to the highly variable ITS2 region. Amplicons were then detected in a simple, colorimetric enzyme immunoassay format (PCR-EIA). DNA sequencing of the ITS1 and ITS2 regions and of the D1-D2 region was also conducted for the differentiation of species by comparative GenBank sequence analysis. The PCR-EIA method was found to be rapid, sensitive, and specific for the identification and differentiation of the most medically important species of Aspergillus. In addition, methods to identify species of Aspergillus by comparative GenBank sequence analysis were found to be more reliable using the ITS1 and ITS2 regions than the D1-D2 regio

Variable Radio Sources in the Galactic Plane

Using three epochs of VLA observations of the Galactic Plane in the first quadrant taken ~15 years apart, we have conducted a search for a population of variable Galactic radio emitters in the flux density range 1-100 mJy at 6 cm. We find 39 variable sources in a total survey area of 23.2 sq deg. Correcting for various selection effects and for the extragalactic variable population of active galactic nuclei, we conclude there are ~1.6 Galactic sources per sq deg which vary by more than 50% on a time scale of years (or shorter). We show that these sources are much more highly variable than extragalactic objects; more than 50% show variability by a factor >2 compared to <10% for extragalactic objects in the same flux density range. We also show that the fraction of variable sources increases toward the Galactic center (another indication that this is a Galactic population), and that the spectral indices of many of these sources are flat or inverted. A small number of the variables are coincident with mid-IR sources and two are coincident with X-ray emitters, but most have no known counterparts at other wavelengths. Intriguingly, one lies at the center of a supernova remnant, while another appears to be a very compact planetary nebula; several are likely to represent activity associated with star formation regions. We discuss the possible source classes which could contribute to the variable cohort and followup observations which could clarify the nature of these sources.Comment: 11 pages, 7 figures; to be published in the Astronomical Journal; data available on MAGPIS website at http://third.ucllnl.org/gps

Evidence for a bound on the lifetime of de Sitter space

Recent work has suggested a surprising new upper bound on the lifetime of de Sitter vacua in string theory. The bound is parametrically longer than the Hubble time but parametrically shorter than the recurrence time. We investigate whether the bound is satisfied in a particular class of de Sitter solutions, the KKLT vacua. Despite the freedom to make the supersymmetry breaking scale exponentially small, which naively would lead to extremely stable vacua, we find that the lifetime is always less than about exp(10^(22)) Hubble times, in agreement with the proposed bound.Comment: 28 page