RESUMEN
The first solids that form as a cooling white dwarf (WD) starts to crystallize are expected to be greatly enriched in actinides. This is because the melting points of WD matter scale as Z^{5/3} and actinides have the largest charge Z. We estimate that the solids may be so enriched in actinides that they could support a fission chain reaction. This reaction could ignite carbon burning and lead to the explosion of an isolated WD in a thermonuclear supernova (SN Ia). Our mechanism could potentially explain SN Ia with sub-Chandrasekhar ejecta masses and short delay times.
RESUMEN
The elastic properties of neutron star crusts are relevant for a variety of currently observable or near-future electromagnetic and gravitational wave phenomena. These phenomena may depend on the elastic properties of nuclear pasta found in the inner crust. We present large-scale classical molecular dynamics simulations where we deform nuclear pasta. We simulate idealized samples of nuclear pasta and describe their breaking mechanism. We also deform nuclear pasta that is arranged into many domains, similar to what is known for the ions in neutron star crusts. Our results show that nuclear pasta may be the strongest known material, perhaps with a shear modulus of 10^{30} ergs/cm^{3} and a breaking strain greater than 0.1.
RESUMEN
Nuclear pasta, with nonspherical shapes, is expected near the base of the crust in neutron stars. Large-scale molecular dynamics simulations of pasta show long lived topological defects that could increase electron scattering and reduce both the thermal and electrical conductivities. We model a possible low-conductivity pasta layer by increasing an impurity parameter Q_{imp}. Predictions of light curves for the low-mass x-ray binary MXB 1659-29, assuming a large Q_{imp}, find continued late time cooling that is consistent with Chandra observations. The electrical and thermal conductivities are likely related. Therefore, observations of late time crust cooling can provide insight on the electrical conductivity and the possible decay of neutron star magnetic fields (assuming these are supported by currents in the crust).
RESUMEN
Coulomb plasmas crystallize in a number of physical systems, such as dusty plasmas, neutron star crusts, and white dwarf cores. The crystal structure of the one-component and binary plasma has received significant attention in the literature, though the less studied multicomponent plasma may be most relevant for many physical systems which contain a large range of particle charges. We report on molecular dynamics simulations of multicomponent plasmas near the melting temperature with mixtures taken to be realistic x-ray burst ash compositions. We quantify the structure of the crystal with the bond order parameters and radial distribution function. Consistent with past work, low charge particles form interstitial defects and we argue that they are in a quasiliquid state within the lattice. The lattice shows screening effects which preserves long-range order despite the large variance in particle charges, which may impact transport properties relevant to astrophysics.
RESUMEN
A number of 21 B. anthracis strains isolated from 16 pustules, 2 blood cultures and 3 cerebrospinal fluids during 2000-2004 were studied for their susceptibility to antibiotics. The antibiosusceptibility testing was performed by disk diffusion method, on Mueller-Hinton agar medium. Two of the studied strains exhibited resistance to penicillins, considered until not long ago as antimicrobial agents of choice for the treatment of anthrax infection. The penicillin resistance explained the difficulties encountered during the treatment of these two cases as well as the fatal evolution in one of them. Both penicillin-resistant strains were subsequently tested, by using "in agar" antibiotic dilution method, in order to determine the minimum inhibitory concentrations (MIC) of the respective strains to penicillin G by the help of a serial antibiotic dilution from 16 microg/ml to 0.0075 microg/ml. The MIC values were 0.5 microg/ml and 4 microg/ml respectively, whereas in case of the standard B. anthracis 34F2 Sterne strain was < 0.015 microg/ml. All the 21 B. anthracis tested strains exhibited resistance to the IIIrd generation cephalosporins, as well as to TMP/STX, but were sensitive to tetracyclines and fluoroquinolones, these sensitivity aspects coming into agreement with the literature data. The strains proved to be also susceptible as follows: 13 strains to macrolides, 15 to rifampicin, 16 to chloramphenicol and all 21 to gentamycin; the last antibiotic can be used in association with fluoroquinolones in the treatment of B. anthracis infections. Fluoroquinolones (i.e. ciprofloxacin) become drugs of choice for the treatment of B. anthracis infections if early administered (within the first 24 hrs), in advance of the germ invasion into the lymph system and septicemia, preventing in this way the bacterial multiplication and production of edemathogenic and lethal toxins.