3,423 research outputs found

    GRB Spikes Could Resolve Stars

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    GRBs vary more rapidly than any other known cosmological phenomena. The lower limits of this variability have not yet been explored. Improvements in detectors would reveal or limit the actual rate of short GRBs. Were microsecond "spike" GRBs to exist and be detectable, they would time-resolve stellar mass objects throughout the universe by their gravitational microlensing effect. Analyzing the time structure of sufficient numbers of GRB spikes would reveal or limit Ī©star\Omega_{star}, Ī©MACHO\Omega_{MACHO}, and/or Ī©baryon\Omega_{baryon}.Comment: 18 pages, 2 figures, in press: ApJ (Letters

    Cāˆ’H Bond Activation by Dicationic Platinum(II) Complexes

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    Double protonolysis of diimine platinum dimethyls [(N-N)PtMe_2] (N-N ā• ArNC(Me)C(Me) ā• NAr) generates dicationic Pt(II) complexes that can activate a variety of Cāˆ’H bonds, liberating 1 equiv of acid and forming organoplatinum species that are moderately stable to the resulting acidic conditions. Ethylbenzenes lead to Ī·^3-benzyl complexes; mechanistic experiments suggest that Ī·^3-benzyl product formation proceeds via Cāˆ’H bond activation at the benzylic methylene position. In some cases Ļ€-arene complexes can be observed, but their role in the Cāˆ’H activation process is not clear. Cyclohexane and 1-pentene react to give Ī·^3-allyl complexes; allylbenzene gives a chelated phenyl-Ī·^2-olefin structure, as determined by X-ray diffraction. No stable Cāˆ’H activation products are obtained from methylbenzenes, benzene itself, or alkanes

    Temperature Effects on Threshold Counterion Concentration to Induce Aggregation of fd Virus

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    We seek to determine the mechanism of like-charge attraction by measuring the temperature dependence of critical divalent counterion concentration (Cc\rm{C_{c}}) for the aggregation of fd viruses. We find that an increase in temperature causes Cc\rm{C_c} to decrease, primarily due to a decrease in the dielectric constant (Ļµ\epsilon) of the solvent. At a constant Ļµ\epsilon, Cc\rm{C_c} is found to increase as the temperature increases. The effects of TT and Ļµ\epsilon on Cc\rm {C_{c}} can be combined to that of one parameter: Bjerrum length (lBl_{B}). Cc\rm{C_{c}} decreases exponentially as lBl_{B} increases, suggesting that entropic effect of counterions plays an important role at the onset of bundle formation.Comment: 12 pages, 3 figure

    Cāˆ’H Bond Activation by Air-Stable [(Diimine)M^(II)(Ī¼_2-OH)]_2^(2+)Dimers (M = Pd, Pt)

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    Air- and water-tolerant Cāˆ’H activation is observed in reactions of [(diimine)Pt(Ī¼_2-OH)]_2^(2+) dimers with allylic and benzylic Cāˆ’H groups. The reactions proceed in good yields under mild conditions. Mechanistic studies indicate that the active species is the monomeric [(diimine)Pt(OH_2)]^(2+) dication. The related palladium species, [(diimine)Pd(Ī¼_2-OH)_2]^(2+), exhibit similar stoichiometric activations and also effect catalytic oxidation of cyclohexene to benzene with molecular oxygen as the terminal oxidant

    Size Ranges of Magnetic Domain States in Tetrataenite

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    Paleomagnetic studies of meteorites provide unique constraints on the evolution of magnetic fields in the early solar system. These studies rely on the identification of magnetic minerals that can retain stable magnetizations over ā‰³4.5 billion years (Ga). The ferromagnetic mineral tetrataenite (Ī³''-Fe0.5Ni0.5) is found in iron, stony-iron and chondrite meteorite groups. Nanoscale intergrowths of tetrataenite have been shown to carry records of paleomagnetic fields, although the effect of magnetostatic interactions on their magnetic remanence acquisition remains to be fully understood. Tetrataenite can also occur as isolated, non-interacting, nanoscale grains in many meteorite groups, although the paleomagnetic potential of these grains is particularly poorly understood. Here, we aim to improve our understanding of tetrataenite magnetization to refine our knowledge of existing paleomagnetic analyses and broaden the spectrum of meteorite groups that can be used for future paleomagnetic studies. We present the results of analytical calculations and micromagnetic modeling of isolated tetrataenite grains with various geometries. We find that tetrataenite forms a stable single domain state at grain lengths between 6 and āˆ¼160 nm dependent on its elongation. It also possesses a magnetization resistant to viscous remagnetization over the lifetime of the solar system at 293 K. At larger grain sizes, tetrataenite's lowest energy state is a lamellar two-domain state, stable at Ga-scale timescales. Unlike many other magnetic minerals, tetrataenite does not form a single-vortex domain state due to its large uniaxial anisotropy. Our results show that single domain and two-domain tetrataenite grains carry an extremely stable magnetization and therefore are promising for paleomagnetic studies

    Computational, Integrative, and Comparative Methods for the Elucidation of Genetic Coexpression Networks

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    Gene expression microarray data can be used for the assembly of genetic coexpression network graphs. Using mRNA samples obtained from recombinant inbred Mus musculus strains, it is possible to integrate allelic variation with molecular and higher-order phenotypes. The depth of quantitative genetic analysis of microarray data can be vastly enhanced utilizing this mouse resource in combination with powerful computational algorithms, platforms, and data repositories. The resulting network graphs transect many levels of biological scale. This approach is illustrated with the extraction of cliques of putatively coregulated genes and their annotation using gene ontology analysis and cis-regulatory element discovery. The causal basis for coregulation is detected through the use of quantitative trait locus mapping

    Basal autophagy induction without AMP-activated protein kinase under low glucose conditions

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    When ATP levels in a cell decrease, various homeostatic intracellular mechanisms initiate attempts to restore ATP levels. As a prominent energy sensor, AMP-activated protein kinase (AMPK) represents one molecular gauge that links energy levels to regulation of anabolic and catabolic processes to restore energy balance. Although pharmacological studies have suggested that an AMPK activator, AICAR (5-aminoimidazole-4-carboxamide ribonucleoside) may link AMPK activation to autophagy, a process that can provide short-term energy within the cell, AICAR can have AMPK-independent effects. Therefore, using a genetic-based approach we investigated the role of AMPK in cellular energy balance. We demonstrate that genetically altered cells, mouse embryonic fibroblasts (MEFs), lacking functional AMPK, display altered energy balance under basal conditions and die prematurely under low glucose-serum starvation challenge. These AMPK mutant cells appear to be abnormally reliant on autophagy under low glucose basal conditions, and therefore cannot rely further on autophagy like wild-type cells during further energetic stress and instead undergo apoptosis. This data suggests that AMPK helps regulate basal energy levels under low glucose. Further, AMPK mutant cells show increased basal phosphorylation of p53 at serine 15, a residue phosphorylated under glucose deprivation. We propose that cells lacking AMPK function have altered p53 activity that may help sensitize these cells to apoptosis under energetic stress
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