5,104 research outputs found

    Nonlinear AC resistivity in s-wave and d-wave disordered granular superconductors

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    We model s-wave and d-wave disordered granular superconductors with a three-dimensional lattice of randomly distributed Josephson junctions with finite self-inductance. The nonlinear ac resistivity of these systems was calculated using Langevin dynamical equations. The current amplitude dependence of the nonlinear resistivity at the peak position is found to be a power law characterized by exponent α\alpha. The later is not universal but depends on the self-inductance and current regimes. In the weak current regime α\alpha is independent of the self-inductance and equal to 0.5 or both of s- and d-wave materials. In the strong current regime this exponent depends on the screening. We find α≈1\alpha \approx 1 for some interval of inductance which agrees with the experimental finding for d-wave ceramic superconductors.Comment: 4 pages, 5 figures, to appear in Phys. Rev. Let

    Transverse depinning and melting of a moving vortex lattice in driven periodic Josephson junction arrays

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    We study the effect of thermal fluctuations in a vortex lattice driven in the periodic pinning of a Josephson junction array. The phase diagram current (II) vs. temperature (TT) is studied. Above the critical current Ic(T)I_c(T) we find a moving vortex lattice (MVL) with anisotropic Bragg peaks. For large currents I≫Ic(T)I\gg I_c(T), there is a melting transition of the MVL at TM(I)T_M(I). When applying a small transverse current to the MVL, there is no dissipation at low TT. We find an onset of transverse vortex motion at a transverse depinning temperature Ttr(I)<TM(I)T_{tr}(I)<T_M(I).Comment: 4 pages, 4 figures, Figure 2 changed, added new reference

    Nonlinear field theories during homogeneous spatial dilation

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    The effect of a uniform dilation of space on stochastically driven nonlinear field theories is examined. This theoretical question serves as a model problem for examining the properties of nonlinear field theories embedded in expanding Euclidean Friedmann-Lema\^{\i}tre-Robertson-Walker metrics in the context of cosmology, as well as different systems in the disciplines of statistical mechanics and condensed matter physics. Field theories are characterized by the speed at which they propagate correlations within themselves. We show that for linear field theories correlations stop propagating if and only if the speed at which the space dilates is higher than the speed at which correlations propagate. The situation is in general different for nonlinear field theories. In this case correlations might stop propagating even if the velocity at which space dilates is lower than the velocity at which correlations propagate. In particular, these results imply that it is not possible to characterize the dynamics of a nonlinear field theory during homogeneous spatial dilation {\it a priori}. We illustrate our findings with the nonlinear Kardar-Parisi-Zhang equation

    Full capacitance-matrix effects in driven Josephson-junction arrays

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    We study the dynamic response to external currents of periodic arrays of Josephson junctions, in a resistively capacitively shunted junction (RCSJ) model, including full capacitance-matrix effects}. We define and study three different models of the capacitance matrix Cr⃗,r⃗′C_{\vec{r},\vec{r}'}: Model A includes only mutual capacitances; Model B includes mutual and self capacitances, leading to exponential screening of the electrostatic fields; Model C includes a dense matrix Cr⃗,r⃗′C_{\vec{r},\vec{r}'} that is constructed approximately from superposition of an exact analytic solution for the capacitance between two disks of finite radius and thickness. In the latter case the electrostatic fields decay algebraically. For comparison, we have also evaluated the full capacitance matrix using the MIT fastcap algorithm, good for small lattices, as well as a corresponding continuum effective-medium analytic evaluation of a finite voltage disk inside a zero-potential plane. In all cases the effective Cr⃗,r⃗′C_{\vec{r},\vec{r}'} decays algebraically with distance, with different powers. We have then calculated current voltage characteristics for DC+AC currents for all models. We find that there are novel giant capacitive fractional steps in the I-V's for Models B and C, strongly dependent on the amount of screening involved. We find that these fractional steps are quantized in units inversely proportional to the lattice sizes and depend on the properties of Cr⃗,r⃗′C_{\vec{r},\vec{r}'}. We also show that the capacitive steps are not related to vortex oscillations but to localized screened phase-locking of a few rows in the lattice. The possible experimental relevance of these results is also discussed.Comment: 12 pages 18 Postscript figures, REVTEX style. Paper to appear in July 1, Vol. 58, Phys. Rev. B 1998 All PS figures include

    Consideraciones sobre la dinámica geomorfológica actual de laderas semiáridas de la Depresión del Ebro: el caso de la Val de las Lenas (término municipal de María de Huerva, Zaragoza, España)

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    [Resumen] En este trabajo se realiza una aproximación al funcionamiento geomorfológico actual de las vales del semiárido aragonés. Las investigaciones contemplan sucesivas aproximaciones, en las que se analizarán: (1) la evolución de humedad en el suelo en diferentes profundidades y posiciones de ladera, (2) las variaciones de la textura del depósito y (3) la simulación de lluvia. Los resultados indican la posible existencia de un funcionamiento hidrológico dislocado a lo largo de la ladera entre el talud superior y los niveles basales. A lo largo del relleno, además, la franja superior parece depender hidrológicamente de su proximidad al talud rocoso adyacente (funcionamiento alóctono), mientras que el depósito de val parece comportarse hidrológicmente de manera autóctona. Entre las partes altas y bajas del relleno de val se aprecia una inversión de las condiciones hídricas que definen su potencial biológico, cuyo reparto espacial es inverso al esperado.[Abstract] We have studied the geomorphological behaviour of slope in a semiarid landscape (NE inland Spain). The approach have been done by the analysis of soil water evolution, particle size analysis and rainfall simulation from top to bottom of slope. Results suggest the posibility of hidrological compartimentation between upper free face and talus; talus is not homogeneous, and there exist a strip in the contact zone with upper free face which change the hidrological regime from upper to lower part of talus

    Hydrodynamic approach to the evolution of cosmological structures

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    A hydrodynamic formulation of the evolution of large-scale structure in the Universe is presented. It relies on the spatially coarse-grained description of the dynamical evolution of a many-body gravitating system. Because of the assumed irrelevance of short-range (``collisional'') interactions, the way to tackle the hydrodynamic equations is essentially different from the usual case. The main assumption is that the influence of the small scales over the large-scale evolution is weak: this idea is implemented in the form of a large-scale expansion for the coarse-grained equations. This expansion builds a framework in which to derive in a controlled manner the popular ``dust'' model (as the lowest-order term) and the ``adhesion'' model (as the first-order correction). It provides a clear physical interpretation of the assumptions involved in these models and also the possibility to improve over them.Comment: 14 pages, 3 figures. Version to appear in Phys. Rev.

    Is the Fast Evolution Scenario for Virialized Compact Groups Really Compelling? The Role of a Dark Massive Group Halo

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    We report on results of N-body simulations aimed at testing the hypothesis that galaxies in X-ray emitting (i.e., virialized) Compact Groups are not tidally stripped when they are embedded in a common, massive, quiescent dark matter halo. To disentangle the effects of interactions from spurious effects due to an incorrect choice of the initial galaxy model configurations, these have been chosen to be tidally-limited King spheres, representing systems in quasi-equilibrium within the tidal field of the halo. The potential of the halo has been assumed to be frozen and the braking due to dynamical friction neglected. Our results confirm the hypothesis of low rates of tidal stripping and suggest a scenario for virialized Compact Group evolution in their quiescent phases with only very moderate tidally induced galaxy evolution can be generally expected. This implies the group stability, provided that the dynamical friction timescales in these systems are not much shorter than the Hubble time. We discuss briefly this possibility, in particular taking account of the similarity between the velocity dispersions of a typical virialized Compact Groups and the internal velocity dispersion of typical member galaxies. A number of puzzling observational data on Compact Groups can be easily explained in this framework. Other observations would be better understood as the result of enhanced merging activity in the proto-group environment, leading to virialized Compact Group formation through mergers of lower mass halos, as predicted by hierarchical scenarios of structure formation.Comment: 18 pages, 1 postscript file, 2 tables, to be published in ApJLet

    The Bethe approximation for solving the inverse Ising problem: a comparison with other inference methods

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    The inverse Ising problem consists in inferring the coupling constants of an Ising model given the correlation matrix. The fastest methods for solving this problem are based on mean-field approximations, but which one performs better in the general case is still not completely clear. In the first part of this work, I summarize the formulas for several mean- field approximations and I derive new analytical expressions for the Bethe approximation, which allow to solve the inverse Ising problem without running the Susceptibility Propagation algorithm (thus avoiding the lack of convergence). In the second part, I compare the accuracy of different mean field approximations on several models (diluted ferromagnets and spin glasses) defined on random graphs and regular lattices, showing which one is in general more effective. A simple improvement over these approximations is proposed. Also a fundamental limitation is found in using methods based on TAP and Bethe approximations in presence of an external field.Comment: v3: strongly revised version with new methods and results, 25 pages, 21 figure
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