5,898 research outputs found

    The Multiple Roles of Low Income, Minority Women in the Family and Community: A Qualitative Investigation

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    This longitudinal, ethnographic research study was incepted to investigate service use among families living in poor urban communities. Themes that emerged during data collection focus on the variety of roles played by women, in the home, and in the neighborhood. We identified numerous strengths exhibited by women, that is, roles that help families adapt and survive. Over a two-year period, we spent time with families, in their homes, and in their communities. Not only did the women fulfill multiple roles in the family, but they performed care taking functions within the community as well. A more complete understanding of family and community strengths will help researchers and social service professionals better serve diverse families

    Spin Dependent Fragmentation Functions for Heavy Flavor Baryons and Single Heavy Hyperon Polarization

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    Spin dependent fragmentation functions for heavy flavor quarks to fragment into heavy baryons are calculated in a quark-diquark model. The production of intermediate spin 1/2 and 3/2 excited states is explicity included. Λb\Lambda_b , Λc\Lambda_c and Ξc\Xi_c production rate and polarization at LEP energies are calculated and, where possible, compared with experiment. A different approach, also relying on a heavy quark-diquark model, is proposed for the small momentum transfer inclusive production of polarized heavy flavor hyperons. The predicted Λc\Lambda_c polarization is roughly in agreement with experiment.Comment: LaTeX2e 11 pages with 4 PostScript figures. To be published in Proceedings of the International Workshop ``Symmetries and spin'', Praha-SPIN-200

    The Evolution of Cloud Cores and the Formation of Stars

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    For a number of starless cores, self-absorbed molecular line and column density observations have implied the presence of large-amplitude oscillations. We examine the consequences of these oscillations on the evolution of the cores and the interpretation of their observations. We find that the pulsation energy helps support the cores and that the dissipation of this energy can lead toward instability and star formation. In this picture, the core lifetimes are limited by the pulsation decay timescales, dominated by non-linear mode-mode coupling, and on the order of ~few x 10^5--10^6 yr. Notably, this is similar to what is required to explain the relatively low rate of conversion of cores into stars. For cores with large-amplitude oscillations, dust continuum observations may appear asymmetric or irregular. As a consequence, some of the cores that would be classified as supercritical may be dynamically stable when oscillations are taken into account. Thus, our investigation motivates a simple hydrodynamic picture, capable of reproducing many of the features of the progenitors of stars without the inclusion of additional physical processes, such as large-scale magnetic fields.Comment: 12 pages, 7 figures, submitted to Ap

    New instability of non-extremal black holes: spitting out supertubes

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    We search for stable bound states of non-extremal rotating three-charge black holes in five dimensions (Cvetic-Youm black holes) and supertubes. We do this by studying the potential of supertube probes in the non-extremal black hole background and find that generically the marginally bound state of the supersymmetric limit becomes metastable and disappears with non-extremality (higher temperature). However near extremality there is a range of parameters allowing for stable bound states, which have lower energy than the supertube-black hole merger. Angular momentum is crucial for this effect. We use this setup in the D1-D5 decoupling limit to map a thermodynamic instability of the CFT (a new phase which is entropically dominant over the black hole phase) to a tunneling instability of the black hole towards the supertube-black hole bound state. This generalizes the results of ArXiv:1108.0411 [hep-th], which mapped an entropy enigma in the bulk to the dual CFT in a supersymmetric setup.Comment: 28 pages + appendix, 15 figures, v2: References added, typos corrected. Version published in JHE

    A (Running) Bolt for New Reasons

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    We construct a four-parameter family of smooth, horizonless, stationary solutions of ungauged five-dimensional supergravity by using the four-dimensional Euclidean Schwarzschild metric as a base space and "magnetizing" its bolt. We then generalize this to a five-parameter family based upon the Euclidean Kerr-Taub-Bolt. These "running Bolt" solutions are necessarily non-static. They also have the same charges and mass as a non-extremal black hole with a classically-large horizon area. Moreover, in a certain regime their mass can decrease as their charges increase. The existence of these solutions supports the idea that the singularities of non-extremal black holes are resolved by low-mass modes that correct the singularity of the classical black hole solution on large (horizon-sized) scales.Comment: 25 pages, 3 figures, LaTeX; v2: minor changes, references adde

    Quantitative studies on the interaction of concanavalin A, the carbohydrate-binding protein of the jack bean, with model carbohydrate-protein conjugates

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    The interaction of concanavalin A with a comprehensive series of carbohydrate-bovine serum albumin comjugates was investigated by agar gel diffusion and quantitative precipitation techniques. These studies showed that when conjugated to bovine serum albumin, those sugars which inhibited concanavalin A-polysaccharide interaction formed a precipitate with concanavalin A. The unexpected reactivity of the p-phenylazo [ss]--glucopyranoside-bovine serum albumin conjugate is rationalized on the basis of inhibition data employing several aryl and alkylglycosides.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/33889/1/0000154.pd

    The Nuts and Bolts of Einstein-Maxwell Solutions

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    We find new non-supersymmetric solutions of five-dimensional ungauged supergravity coupled to two vector multiplets. The solutions are regular, horizonless and have the same asymptotic charges as non-extremal charged black holes. An essential ingredient in our construction is a four-dimensional Euclidean base which is a solution to Einstein-Maxwell equations. We construct stationary solutions based on the Euclidean dyonic Reissner-Nordstrom black hole as well as a six-parameter family with a dyonic Kerr-Newman-NUT base. These solutions can be viewed as compactifications of eleven-dimensional supergravity on a six-torus and we discuss their brane interpretation.Comment: 29 pages, 3 figure

    Immunochemical studies on a laminaribiosyl-azoprotein conjugate

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    Laminaribiose () was coupled to bovine serum albumin (BSA) by an azophenyl linkage to provide the synthetic antigen BSA-p-phenylazo-[beta]-laminaribioside. The behavior of antisera prepared in rabbits immunized with the [beta]-laminaribiosyl conjugate was examined by immunodiffusion, quantitative precipitation and hapten inhibition. Anticonjugate absorbed with carrier protein showed the greatest reactivity with the homologous [beta]-laminaribiosyl-BSA antigen, but also showed some cross precipitation with [beta]-cellobiosyl, [beta]-sophorosyl and [beta]-gentiobiosyl-BSA conjugates. Glucobioses linked through the [beta]-(1 --> 2), [beta]-(1 --> 3), [beta]-(1 --> 4) and [beta]-(1 --> 6) positions, as well as laminaridextrins and tri and tetrasaccharides of [beta]-linked glucose possessing a laminaribiose moiety either at a nonreducing end location or at a subterminal location, were assayed for their ability to inhibit antilaminaribioside precipitation. Hapten inhibition data showed anticonjugate a possess a high degree of specificity directed against the terminal nonreducing [beta]-laminaribiosyl end group.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/32752/1/0000121.pd
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