99 research outputs found

    Generation of Porous Particle Structures using the Void Expansion Method

    Full text link
    The newly developed "void expansion method" allows for an efficient generation of porous packings of spherical particles over a wide range of volume fractions using the discrete element method. Particles are randomly placed under addition of much smaller "void-particles". Then, the void-particle radius is increased repeatedly, thereby rearranging the structural particles until formation of a dense particle packing. The structural particles' mean coordination number was used to characterize the evolving microstructures. At some void radius, a transition from an initially low to a higher mean coordination number is found, which was used to characterize the influence of the various simulation parameters. For structural and void-particle stiffnesses of the same order of magnitude, the transition is found at constant total volume fraction slightly below the random close packing limit. For decreasing void-particle stiffness the transition is shifted towards a smaller void-particle radius and becomes smoother.Comment: 9 pages, 8 figure

    The Influence of the Degree of Heterogeneity on the Elastic Properties of Random Sphere Packings

    Full text link
    The macroscopic mechanical properties of colloidal particle gels strongly depend on the local arrangement of the powder particles. Experiments have shown that more heterogeneous microstructures exhibit up to one order of magnitude higher elastic properties than their more homogeneous counterparts at equal volume fraction. In this paper, packings of spherical particles are used as model structures to computationally investigate the elastic properties of coagulated particle gels as a function of their degree of heterogeneity. The discrete element model comprises a linear elastic contact law, particle bonding and damping. The simulation parameters were calibrated using a homogeneous and a heterogeneous microstructure originating from earlier Brownian dynamics simulations. A systematic study of the elastic properties as a function of the degree of heterogeneity was performed using two sets of microstructures obtained from Brownian dynamics simulation and from the void expansion method. Both sets cover a broad and to a large extent overlapping range of degrees of heterogeneity. The simulations have shown that the elastic properties as a function of the degree of heterogeneity are independent of the structure generation algorithm and that the relation between the shear modulus and the degree of heterogeneity can be well described by a power law. This suggests the presence of a critical degree of heterogeneity and, therefore, a phase transition between a phase with finite and one with zero elastic properties.Comment: 8 pages, 6 figures; Granular Matter (published online: 11. February 2012

    Measurement of the Eta Production in Proton Proton Collisions with the COSY Time of Flight Spectrometer

    Get PDF
    The reaction pp -> pp eta was measured at excess energies of 15 and 41 MeV at an external target of the Juelich Cooler Synchrotron COSY with the Time of Flight Spectrometer. About 25000 events were measured for the excess energy of 15 MeV and about 8000 for 41 MeV. Both protons of the process pp eta were detected with an acceptance of nearly 100% and the eta was reconstructed by the missing mass technique. For both excess energies the angular distributions are found to be nearly isotropic. In the invariant mass distributions strong deviations from the pure phase space distributions are seen.Comment: 15 pages, 14 figures, 4 table

    Single-Pion Production in pp Collisions at 0.95 GeV/c (II)

    Get PDF
    The single-pion production reactions ppdπ+pp\to d\pi^+, ppnpπ+pp\to np\pi^+ and ppppπ0pp\to pp\pi^0 were measured at a beam momentum of 0.95 GeV/c (TpT_p \approx 400 MeV) using the short version of the COSY-TOF spectrometer. The central calorimeter provided particle identification, energy determination and neutron detection in addition to time-of-flight and angle measurements from other detector parts. Thus all pion production channels were recorded with 1-4 overconstraints. Main emphasis is put on the presentation and discussion of the npπ+np\pi^+ channel, since the results on the other channels have already been published previously. The total and differential cross sections obtained are compared to theoretical calculations. In contrast to the ppπ0pp\pi^0 channel we find in the npπ+np\pi^+ channel a strong influence of the Δ\Delta excitation already at this energy close to threshold. In particular we find a (3cos2Θ+1)(3 cos^2\Theta + 1) dependence in the pion angular distribution, typical for a pure s-channel Δ\Delta excitation and identical to that observed in the dπ+d\pi^+ channel. Since the latter is understood by a s-channel resonance in the 1D2^1D_2 pnpn partial wave, we discuss an analogous scenario for the pnπ+pn\pi^+ channel

    Production of ω\omega mesons in proton-proton collisions

    Get PDF
    The cross section for the production of ω\omega mesons in proton-proton collisions has been measured in a previously unexplored region of incident energies. Cross sections were extracted at 92 MeV and 173 MeV excess energy, respectively. The angular distribution of the ω\omega at ϵ\epsilon=173 MeV is strongly anisotropic, demonstrating the importance of partial waves beyond pure s-wave production at this energy.Comment: 12 pages, 4 figures submitted to Physics Letters B v2: figure 1 added, discussion detailing the data analysis, figure 3 (fig. 2 in v1) modified in line styles and systematic errors displayed on dat

    Comparison of Isoscalar Vector Meson Production Cross Sections in Proton-Proton Collisions

    Get PDF
    The reaction ppppω pp\to pp\bf \omega was investigated with the TOF spectrometer, which is an external experiment at the accelerator COSY (Forschungszentrum J\"ulich, Germany). Total as well as differential cross sections were determined at an excess energy of 93MeV93 MeV (pbeam=2950MeV/cp_{beam}=2950 MeV/c). Using the total cross section of (9.0±0.7±1.1)μb(9.0\pm 0.7 \pm1.1) \mu b for the reaction ppppω pp\to pp\omega determined here and existing data for the reaction ppppϕpp\to pp\bf \phi, the ratio Rϕ/ω=σϕ/σω\mathcal{R}_{\phi/\omega}=\sigma_\phi/\sigma_\omega turns out to be significantly larger than expected by the Okubo-Zweig-Iizuka (OZI) rule. The uncertainty of this ratio is considerably smaller than in previous determinations. The differential distributions show that the ω\omega production is still dominated by S-wave production at this excess energy, however higher partial waves clearly contribute. A comparison of the measured angular distributions for ω\omega production to published distributions for ϕ\phi production at 83MeV83 MeV shows that the data are consistent with an identical production mechanism for both vector mesons

    On the Production of π+π+\pi^+\pi^+ Pairs in pp Collisions at 0.8 GeV

    Get PDF
    Data accumulated recently for the exclusive measurement of the ppppπ+πpp\to pp\pi^+\pi^- reaction at a beam energy of 0.793 GeV using the COSY-TOF spectrometer have been analyzed with respect to possible events from the ppnnπ+π+pp \to nn\pi^+\pi^+ reaction channel. The latter is expected to be the only ππ\pi\pi production channel, which contains no major contributions from resonance excitation close to threshold and hence should be a good testing ground for chiral dynamics in the ππ\pi\pi production process. No single event has been found, which meets all conditions for being a candidate for the ppnnπ+π+pp \to nn \pi^+\pi^+ reaction. This gives an upper limit for the cross section of 0.16 μ\mub (90% C.L.), which is more than an order of magnitude smaller than the cross sections of the other two-pion production channels at the same incident energy

    Production of Lambda and Sigma^0 hyperons in proton-proton collisions

    Get PDF
    This paper reports results on simultaneous measurements of the reaction channels pp -> pK+\Lambda and pp -> pK+\Sigma^0 at excess energies of 204, 239, and 284 MeV (\Lambda) and 127, 162, and 207 MeV (\Sigma^0). Total and differential cross sections are given for both reactions. It is concluded from the measured total cross sections that the high energy limit of the cross section ratio is almost reached at an excess energy of only about 200 MeV. From the differential distributions observed in the overall CMS as well as in the Jackson and helicity frames, a significant contribution of interfering nucleon resonances to the \Lambda production mechanism is concluded while resonant \Sigma^0-production seems to be of lesser importance and takes place only through specific partial waves of the entrance channel. The data also indicate that kaon exchange plays a minor role in the case of \Lambda- but an important role for \Sigma^0-production. Thus the peculiar energy dependence of the \Lambda-to-\Sigma^0 cross section ratio appears in a new light as its explanation requires more than mere differences between the p\Lambda and the p\Sigma^0 final state interaction. The data provide a benchmark for theoretical models already available or yet to come.Comment: 18 pages, 10 figures; accepted by The European Physical Journal A (EPJ A

    Nuclear Reaction Rates and Primordial 6^6Li

    Get PDF
    We examine the possibility that Big Bang Nucleosynthesis (BBN) may produce non-trivial amounts of 6^6Li. If a primordial component of this isotope could be observed, it would provide a new fundamental test of Big-Bang cosmology, as well as new constraints on the baryon density of the universe. At present, however, theoretical predictions of the primordial 6^6Li abundance are extremely uncertain due to difficulties in both theoretical estimates and experimental determinations of the deuterium-plus-alpha radiative capture reaction cross-section. We also argue that present observational capabilities do not yet allow the detection of primeval 6^6Li in very metal-poor stars of the galactic halo. However, if the critical cross section is towards the upper end of its plausible range, then improvements in 6^6Li detection capabilities may allow the establishment of 6^6Li as another product of BBN. It is also noted that a primordial 6^6Li detection could help resolve current concerns about the extragalactic D/H determination.Comment: 10 pages, REVTeX, 5 PostScript figures with psfig. Submitted to Physical Review
    corecore