Interstitial Electronic Localization

We investigate the ground-state properties of a collection of \textit{N} non-interacting electrons in a macroscopic volume $\Omega$ also containing a crystalline array of \textit{N} spheres of radius $r_c$ each taken as largely impenetrable to electrons and with proximity of neighboring excluding regions playing a key physical role. The sole parameter of this quantum system is the ratio $r_c/r_s$, where $r_s$ is the Wigner- Seitz radius. Two lattices (FCC and BCC) are selected to illustrate the behavior of the system as a function of $r_c/r_s$. As this ratio increases valence electrons localize in the interstitial regions and the relative band-width $\epsilon_F/\epsilon_F^0$ is found to decrease monotonically for both. The system is motivated by the behavior of the alkali metals at significant compression. It accounts for band narrowing, leads to electronic densities with interstitially centered maxima, and can be taken as a model which clearly may be improved upon by perturbation and other methods.Comment: 11 pages, 5 figure

Successful Implementation of the ABCDEF Bundle in the MICU through Interprofessional Collaboration and Teamwork

Earlier this year, members of the medical intensive care unit (MICU) attended an interprofessional workshop that utilized Awakening/Breathing/Choice of Sedation/Delirium/Early Mobility (ABCDE) bundle simulation combined with TeamSTEPPS training to empower care givers to advocate for patient safety while optimizing patient care. The ABCDE bundle is an evidence-based tool designed to implement pain, agitation, and delirium guideline recommendations into routine practice. To further improve patient safety and outcomes and build upon the ABCDE concept, the MICU team developed an interprofession-al practice project by adding routine assessment of need for indwelling Foley catheters to their daily work list, creating the “ABCDEF” bundle

Optimal statistic for detecting gravitational wave signals from binary inspirals with LISA

A binary compact object early in its inspiral phase will be picked up by its nearly monochromatic gravitational radiation by LISA. But even this innocuous appearing candidate poses interesting detection challenges. The data that will be scanned for such sources will be a set of three functions of LISA's twelve data streams obtained through time-delay interferometry, which is necessary to cancel the noise contributions from laser-frequency fluctuations and optical-bench motions to these data streams. We call these three functions pseudo-detectors. The sensitivity of any pseudo-detector to a given sky position is a function of LISA's orbital position. Moreover, at a given point in LISA's orbit, each pseudo-detector has a different sensitivity to the same sky position. In this work, we obtain the optimal statistic for detecting gravitational wave signals, such as from compact binaries early in their inspiral stage, in LISA data. We also present how the sensitivity of LISA, defined by this optimal statistic, varies as a function of sky position and LISA's orbital location. Finally, we show how a real-time search for inspiral signals can be implemented on the LISA data by constructing a bank of templates in the sky positions.Comment: 22 pages, 15 eps figures, Latex, uses iopart style/class files. Based on talk given at the 8th Gravitational Wave Data Analysis Workshop, Milwaukee, USA, December 17-20, 2003. Accepted for publication in Class. Quant. Gra