720 research outputs found

    Gravitational waves from supernova matter

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    We have performed a set of 11 three-dimensional magnetohydrodynamical core collapse supernova simulations in order to investigate the dependencies of the gravitational wave signal on the progenitor's initial conditions. We study the effects of the initial central angular velocity and different variants of neutrino transport. Our models are started up from a 15 solar mass progenitor and incorporate an effective general relativistic gravitational potential and a finite temperature nuclear equation of state. Furthermore, the electron flavour neutrino transport is tracked by efficient algorithms for the radiative transfer of massless fermions. We find that non- and slowly rotating models show gravitational wave emission due to prompt- and lepton driven convection that reveals details about the hydrodynamical state of the fluid inside the protoneutron stars. Furthermore we show that protoneutron stars can become dynamically unstable to rotational instabilities at T/|W| values as low as ~2 % at core bounce. We point out that the inclusion of deleptonization during the postbounce phase is very important for the quantitative GW prediction, as it enhances the absolute values of the gravitational wave trains up to a factor of ten with respect to a lepton-conserving treatment.Comment: 10 pages, 6 figures, accepted, to be published in a Classical and Quantum Gravity special issue for MICRA200

    BlutgefÀsssegmentation in MR-Bildern mittels Aktivkontur-Modellen

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    Stochastic reconstruction of sandstones

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    A simulated annealing algorithm is employed to generate a stochastic model for a Berea and a Fontainebleau sandstone with prescribed two-point probability function, lineal path function, and ``pore size'' distribution function, respectively. We find that the temperature decrease of the annealing has to be rather quick to yield isotropic and percolating configurations. A comparison of simple morphological quantities indicates good agreement between the reconstructions and the original sandstones. Also, the mean survival time of a random walker in the pore space is reproduced with good accuracy. However, a more detailed investigation by means of local porosity theory shows that there may be significant differences of the geometrical connectivity between the reconstructed and the experimental samples.Comment: 12 pages, 5 figure

    Nonequilibrium Phase Transitions in Models of Aggregation, Adsorption, and Dissociation

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    We study nonequilibrium phase transitions in a mass-aggregation model which allows for diffusion, aggregation on contact, dissociation, adsorption and desorption of unit masses. We analyse two limits explicitly. In the first case mass is locally conserved whereas in the second case local conservation is violated. In both cases the system undergoes a dynamical phase transition in all dimensions. In the first case, the steady state mass distribution decays exponentially for large mass in one phase, and develops an infinite aggregate in addition to a power-law mass decay in the other phase. In the second case, the transition is similar except that the infinite aggregate is missing.Comment: Major revision of tex

    Phase Transition in the Takayasu Model with Desorption

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    We study a lattice model where particles carrying different masses diffuse, coalesce upon contact, and also unit masses adsorb to a site with rate qq or desorb from a site with nonzero mass with rate pp. In the limit p=0p=0 (without desorption), our model reduces to the well studied Takayasu model where the steady-state single site mass distribution has a power law tail P(m)∌m−τP(m)\sim m^{-\tau} for large mass. We show that varying the desorption rate pp induces a nonequilibrium phase transition in all dimensions. For fixed qq, there is a critical pc(q)p_c(q) such that if p<pc(q)p<p_c(q), the steady state mass distribution, P(m)∌m−τP(m)\sim m^{-\tau} for large mm as in the Takayasu case. For p=pc(q)p=p_c(q), we find P(m)∌m−τcP(m)\sim m^{-\tau_c} where τc\tau_c is a new exponent, while for p>pc(q)p>p_c(q), P(m)∌exp⁥(−m/m∗)P(m)\sim \exp(-m/m^*) for large mm. The model is studied analytically within a mean field theory and numerically in one dimension.Comment: RevTex, 11 pages including 5 figures, submitted to Phys. Rev.

    Unified View of Scaling Laws for River Networks

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    Scaling laws that describe the structure of river networks are shown to follow from three simple assumptions. These assumptions are: (1) river networks are structurally self-similar, (2) single channels are self-affine, and (3) overland flow into channels occurs over a characteristic distance (drainage density is uniform). We obtain a complete set of scaling relations connecting the exponents of these scaling laws and find that only two of these exponents are independent. We further demonstrate that the two predominant descriptions of network structure (Tokunaga's law and Horton's laws) are equivalent in the case of landscapes with uniform drainage density. The results are tested with data from both real landscapes and a special class of random networks.Comment: 14 pages, 9 figures, 4 tables (converted to Revtex4, PRE ref added

    Kang-Redner Anomaly in Cluster-Cluster Aggregation

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    The large time, small mass, asymptotic behavior of the average mass distribution \pb is studied in a dd-dimensional system of diffusing aggregating particles for 1≀d≀21\leq d \leq 2. By means of both a renormalization group computation as well as a direct re-summation of leading terms in the small reaction-rate expansion of the average mass distribution, it is shown that \pb \sim \frac{1}{t^d} (\frac{m^{1/d}}{\sqrt{t}})^{e_{KR}} for mâ‰Ștd/2m \ll t^{d/2}, where eKR=Ï”+O(Ï”2)e_{KR}=\epsilon +O(\epsilon ^2) and Ï”=2−d\epsilon =2-d. In two dimensions, it is shown that \pb \sim \frac{\ln(m) \ln(t)}{t^2} for mâ‰Șt/ln⁥(t) m \ll t/ \ln(t). Numerical simulations in two dimensions supporting the analytical results are also presented.Comment: 11 pages, 6 figures, Revtex
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