120 research outputs found

    μ-DSMC: A general viscosity method for rarefied flow

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    A modified DSMC method for rarefied flows is described, by which any viscosity law mu = mu(T) may be simulated, including experimental data directly. The collision cross-section of a simple collision model is made to vary from cell to cell, based on the time-averaged cell temperature and the required viscosity at that temperature. The new method is tested in two different flows: high speed Couette flow and a plane 1D shock. For Couette flow, the shear stress and heat transfer, calculated from the velocity distribution, agree with the theoretical values calculated from the flow gradients and the theoretical transport coefficients. For the 1D shock, the new method is compared with the generalized hard sphere (GHS) model. The new method produces profiles of density and temperature which are generally indistinguishable from the GHS results except for a deviation in the Tx temperature component in a small region ahead of the shock. For the worst case the deviation is 4.6%, but it can be reduced by basing the imposed viscosity on the maximum component of kinetic temperature rather than the mean kinetic temperature. The new method is shown to be insensitive to the number of simulator particles used in each cell. Three translational degrees of freedom are considered. However, because mu-DSMC is based on a hard sphere or VHS cross-section, it is compatible with the most commonly used Borgnakke-Larsen model for translational-rotational energy exchange

    The Ruderman-Kittel-Kasuya-Yosida (RKKY) interaction across a tunneling junction out of equilibrium

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    The Ruderman-Kittel-Kasuya-Yosida (RKKY) interaction between two magnetic ss-dd spin impurities across a tunneling junction is studied when the system is driven out of equilibrium through biasing the junction. The nonequilibrium situation is handled with the Keldysh time-loop perturbation formalism in conjunction with appropriate coupling methods for tunneling systems due to Caroli and Feuchtwang. We find that the presence of a nonequilibrium bias across the junction leads to an interference of several fundamental oscillations, such that in this tunneling geometry, it is possible to tune the interaction between ferromagnetic and antiferromagnetic coupling at a fixed impurity configuration, simply by changing the bias across the junction. Furthermore, it is shown that the range of the RKKY interaction is altered out of equilibrium, such that in particular the interaction energy between two slabs of spins scales extensively with the thickness of the slabs in the presence of an applied bias.Comment: 38 pages revtex preprint; 5 postscript figures; submitted to Phys. Rev.

    Counterion Condensation and Fluctuation-Induced Attraction

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    We consider an overall neutral system consisting of two similarly charged plates and their oppositely charged counterions and analyze the electrostatic interaction between the two surfaces beyond the mean-field Poisson-Boltzmann approximation. Our physical picture is based on the fluctuation-driven counterion condensation model, in which a fraction of the counterions is allowed to ``condense'' onto the charged plates. In addition, an expression for the pressure is derived, which includes fluctuation contributions of the whole system. We find that for sufficiently high surface charges, the distance at which the attraction, arising from charge fluctuations, starts to dominate can be large compared to the Gouy-Chapmann length. We also demonstrate that depending on the valency, the system may exhibit a novel first-order binding transition at short distances.Comment: 15 pages, 8 figures, to appear in PR

    The Physics of Star Cluster Formation and Evolution

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    © 2020 Springer-Verlag. The final publication is available at Springer via https://doi.org/10.1007/s11214-020-00689-4.Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is transformed to turbulence with stars forming from cores fed by filaments. In the most compact regions, stellar feedback is least effective in removing the gas and stars may form very efficiently. These are also the regions where, in high-mass clusters, ejecta from some kind of high-mass stars are effectively captured during the formation phase of some of the low mass stars and effectively channeled into the latter to form multiple populations. Star formation epochs in star clusters are generally set by gas flows that determine the abundance of gas in the cluster. We argue that there is likely only one star formation epoch after which clusters remain essentially clear of gas by cluster winds. Collisional dynamics is important in this phase leading to core collapse, expansion and eventual dispersion of every cluster. We review recent developments in the field with a focus on theoretical work.Peer reviewe

    Geographical and temporal distribution of SARS-CoV-2 clades in the WHO European Region, January to June 2020

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    We show the distribution of SARS-CoV-2 genetic clades over time and between countries and outline potential genomic surveillance objectives. We applied three available genomic nomenclature systems for SARS-CoV-2 to all sequence data from the WHO European Region available during the COVID-19 pandemic until 10 July 2020. We highlight the importance of real-time sequencing and data dissemination in a pandemic situation. We provide a comparison of the nomenclatures and lay a foundation for future European genomic surveillance of SARS-CoV-2.Peer reviewe

    Characteristics of the nuclear (18S, 5.8S, 28S and 5S) and mitochondrial (12S and 16S) rRNA genes of Apis mellifera (Insecta: Hymenoptera): structure, organization, and retrotransposable elements

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    As an accompanying manuscript to the release of the honey bee genome, we report the entire sequence of the nuclear (18S, 5.8S, 28S and 5S) and mitochondrial (12S and 16S) ribosomal RNA (rRNA)-encoding gene sequences (rDNA) and related internally and externally transcribed spacer regions of Apis mellifera (Insecta: Hymenoptera: Apocrita). Additionally, we predict secondary structures for the mature rRNA molecules based on comparative sequence analyses with other arthropod taxa and reference to recently published crystal structures of the ribosome. In general, the structures of honey bee rRNAs are in agreement with previously predicted rRNA models from other arthropods in core regions of the rRNA, with little additional expansion in non-conserved regions. Our multiple sequence alignments are made available on several public databases and provide a preliminary establishment of a global structural model of all rRNAs from the insects. Additionally, we provide conserved stretches of sequences flanking the rDNA cistrons that comprise the externally transcribed spacer regions (ETS) and part of the intergenic spacer region (IGS), including several repetitive motifs. Finally, we report the occurrence of retrotransposition in the nuclear large subunit rDNA, as R2 elements are present in the usual insertion points found in other arthropods. Interestingly, functional R1 elements usually present in the genomes of insects were not detected in the honey bee rRNA genes. The reverse transcriptase products of the R2 elements are deduced from their putative open reading frames and structurally aligned with those from another hymenopteran insect, the jewel wasp Nasonia (Pteromalidae). Stretches of conserved amino acids shared between Apis and Nasonia are illustrated and serve as potential sites for primer design, as target amplicons within these R2 elements may serve as novel phylogenetic markers for Hymenoptera. Given the impending completion of the sequencing of the Nasonia genome, we expect our report eventually to shed light on the evolution of the hymenopteran genome within higher insects, particularly regarding the relative maintenance of conserved rDNA genes, related variable spacer regions and retrotransposable elements

    Calcium and phosphorus supplementation in grazing lactating Zebu cows, in Iringa District, Tanzania

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    Tanzania Journal of Agricultural Sciences 2002, Vol.5(1) : 71-76The effects of dietary supplementation with dicalcium phosphate containing 10 g calcium and 8 g phosphorus on plasma total calcium inorganic phosphate, body condition score and milk yield were studied for 42 days, during the dry season of 1997 in forty grazing, lactating Zebu cows, in lringa region, Tanzania. The animals were allocated to two groups: one control group (T1) comprising off fifteen cows and a supplementation groUp (T2) comprising of twenty five cows. Dicalcium phosphate supplementation was done twice per week. Blood samples were collected before supplementation and at the engd of experimental period. Total milk yield and body condition of the animals were also recorded. Supplemented cows had higher (P< 0.001) mean plasma calcium and inorganic phosphate (1.30 mmol/Ca and 2. 08 mmol P/l) than the control cows (1.08 mmol/Ca and 1.58 mmol P/l). Supplemented cows, had a better (P<0. 0001) body condition score and produced more milk (3. 10 BCS and 181 kg) than control cows (2.63 BCS and 149 kg) and total 42 days milk yield (149 vs 181 kg). It is concluded that low plasma calcium and inorganic phosphate may be a problem to Zebu cows and that decalcium phosphate can provide a boost to plasma Ca and Pi ,during the dry seaso
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