49,800 research outputs found

    Primary Amoebic (Naegleria fowleri) Meningoencephalitis Presenting as Status Epilepticus

    Get PDF
    Primary amebic meningoencephalitis (PAM) is a rare entity. Usual presenting features are fever, headache and seizures with meningeal signs and this disease carries high mortality rate. We present a case report of PAM presenting as status epilepticus

    Firing Pin Scrape Marks and the Identification of Firearms

    Get PDF

    Turbulence and Mixing in the Intracluster Medium

    Full text link
    The intracluster medium (ICM) is stably stratified in the hydrodynamic sense with the entropy ss increasing outwards. However, thermal conduction along magnetic field lines fundamentally changes the stability of the ICM, leading to the "heat-flux buoyancy instability" when dT/dr>0dT/dr>0 and the "magnetothermal instability" when dT/dr<0dT/dr<0. The ICM is thus buoyantly unstable regardless of the signs of dT/drdT/dr and ds/drds/dr. On the other hand, these temperature-gradient-driven instabilities saturate by reorienting the magnetic field (perpendicular to r^\hat{\bf r} when dT/dr>0dT/dr>0 and parallel to r^\hat{\bf r} when dT/dr<0dT/dr<0), without generating sustained convection. We show that after an anisotropically conducting plasma reaches this nonlinearly stable magnetic configuration, it experiences a buoyant restoring force that resists further distortions of the magnetic field. This restoring force is analogous to the buoyant restoring force experienced by a stably stratified adiabatic plasma. We argue that in order for a driving mechanism (e.g, galaxy motions or cosmic-ray buoyancy) to overcome this restoring force and generate turbulence in the ICM, the strength of the driving must exceed a threshold, corresponding to turbulent velocities 10100km/s\gtrsim 10 -100 {km/s}. For weaker driving, the ICM remains in its nonlinearly stable magnetic configuration, and turbulent mixing is effectively absent. We discuss the implications of these findings for the turbulent diffusion of metals and heat in the ICM.Comment: 8 pages, 2 figs., submitted to the conference proceedings of "The Monster's Fiery Breath;" a follow up of arXiv:0901.4786 focusing on the general mixing properties of the IC

    Agricultural growth and structural changes in the Punjab economy: an input-output analysis

    Get PDF
    Agriculture Economic aspects India Punjab., Punjab (India) Economic conditions., Input-output analysis India Punjab.,

    A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory

    Get PDF
    A new parameterization for an effective non-linear Lagrangian density of relativistic mean field (RMF) theory is proposed, which is able to provide an excellent description not only for the properties of stable nuclei but also for those far from the valley of beta-stability. In addition recently measured superdeformed mimima in the Hg-region are reproduced with high accuracy.Comment: 8 pages, Latex, 1 ps figur

    Nuclear Breathing Mode in the Relativistic Mean Field Theory

    Full text link
    The breathing-mode giant monopole resonance is studied within the framework of the relativistic mean-field (RMF) theory. Using a broad range of parameter sets, an analysis of constrained incompressibility and excitation energy of isoscalar monopole states in finite nuclei is performed. It is shown that the non-linear scalar self-interaction and the resulting surface properties influence the breathing-mode considerably. It is observed that dynamical surface properties respond differently in the RMF theory than in the Skyrme approach. A comparison is made with the incompressibility derived from the semi-infinite nuclear matter and with constrained nonrelativistic Skyrme Hartree-Fock calculaions.Comment: Latex (12 pages) and 3 figures (available upon request) J. Phys. G (in press
    corecore