4,921 research outputs found

    An Introduction to Breakdown Phenomena in Disordered Systems

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    The rupture of a medium under stress typifies breakdown phenomena. More generally, the latter encompass the dynamics of systems of many interacting elements governed by the interplay of a driving force with a pinning disorder, resulting in a macroscopic transition. A simple mean-field formalism incorporating these features is presented and applied to systems representative of fracture phenomena, social dilemmas, and magnets out of equilibrium. The similarities and differences in the corresponding mathematical structures are emphasized. The solutions are best obtained from a graphical method, from which very general conclusions may be drawn. In particular, the various classes of disorder distribution are treated without reference to a particular analytical or numerical form, and are found to lead to qualitatively different transitions. Finally, the notion of effective (or phenomenological) theory is introduced and illustrated for non-equilibrium disordered magnets.Comment: Pedagogical article published as part of a special issue on thermodynamics and statistical physics; 20 page

    Electron cyclotron maser emission mode coupling to the z-mode on a longitudinal density gradient in the context of solar type III bursts

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    Copyright 2012 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. This article appeared in Physics of Plasmas 19, 110702 (2012) and may be found at .supplemental material at http://astro.qmul.ac.uk/~tsiklauri/sp.htmlsupplemental material at http://astro.qmul.ac.uk/~tsiklauri/sp.htm

    Field-dependent diamagnetic transition in magnetic superconductor Sm1.85Ce0.15CuO4ySm_{1.85} Ce_{0.15} Cu O_{4-y}

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    The magnetic penetration depth of single crystal Sm1.85Ce0.15CuO4y\rm{Sm_{1.85}Ce_{0.15}CuO_{4-y}} was measured down to 0.4 K in dc fields up to 7 kOe. For insulating Sm2CuO4\rm{Sm_2CuO_4}, Sm3+^{3+} spins order at the N\'{e}el temperature, TN=6T_N = 6 K, independent of the applied field. Superconducting Sm1.85Ce0.15CuO4y\rm{Sm_{1.85}Ce_{0.15}CuO_{4-y}} (Tc23T_c \approx 23 K) shows a sharp increase in diamagnetic screening below T(H)T^{\ast}(H) which varied from 4.0 K (H=0H = 0) to 0.5 K (H=H = 7 kOe) for a field along the c-axis. If the field was aligned parallel to the conducting planes, TT^{\ast} remained unchanged. The unusual field dependence of TT^{\ast} indicates a spin freezing transition that dramatically increases the superfluid density.Comment: 4 pages, RevTex

    The effect of electron beam pitch angle and density gradient on solar type III radio bursts

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    Copyright 2012 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. This article appeared in Physics of Plasmas 19, 112903 (2012) and may be found at .supplemental material at http://astro.qmul.ac.uk/~tsiklauri/sp.htmlsupplemental material at http://astro.qmul.ac.uk/~tsiklauri/sp.htm

    Evolution of Universe to the present inert phase

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    We assume that current state of the Universe can be described by the Inert Doublet Model, containing two scalar doublets, one of which is responsible for EWSB and masses of particles and the second one having no couplings to fermions and being responsible for dark matter. We consider possible evolutions of the Universe to this state during cooling down of the Universe after inflation. We found that in the past Universe could pass through phase states having no DM candidate. In the evolution via such states in addition to a possible EWSB phase transition (2-nd order) the Universe sustained one 1-st order phase transition or two phase transitions of the 2-nd order.Comment: 19 pages, 3 figure

    Chain length dependence of the polymer-solvent critical point parameters

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    We report grand canonical Monte Carlo simulations of the critical point properties of homopolymers within the Bond Fluctuation model. By employing Configurational Bias Monte Carlo methods, chain lengths of up to N=60 monomers could be studied. For each chain length investigated, the critical point parameters were determined by matching the ordering operator distribution function to its universal fixed-point Ising form. Histogram reweighting methods were employed to increase the efficiency of this procedure. The results indicate that the scaling of the critical temperature with chain length is relatively well described by Flory theory, i.e. \Theta-T_c\sim N^{-0.5}. The critical volume fraction, on the other hand, was found to scale like \phi_c\sim N^{-0.37}, in clear disagreement with the Flory theory prediction \phi_c\sim N^{-0.5}, but in good agreement with experiment. Measurements of the chain length dependence of the end-to-end distance indicate that the chains are not collapsed at the critical point.Comment: 13 Pages Revtex, 9 epsf embedded figs. gzipped tar file. To appear in J. Chem. Phy

    Complete description of polarization effects in e^+e^- pair production by a photon in the field of a strong laser wave

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    We consider production of a e^+e^- pair by a high-energy photon in the field of a strong laser wave. A probability of this process for circularly or linearly polarized laser photons and for arbitrary polarization of all other particles is calculated. We obtain the complete set of functions which describe such a probability in a compact invariant form. Besides, we discuss in some detail the polarization effects in the kinematics relevant to the problem of electron-photon conversion at photon-photon and electron-photon colliders.Comment: 14 pages, 8 figure

    Detecting photon-photon scattering in vacuum at exawatt lasers

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    In a recent paper, we have shown that the QED nonlinear corrections imply a phase correction to the linear evolution of crossing electromagnetic waves in vacuum. Here, we provide a more complete analysis, including a full numerical solution of the QED nonlinear wave equations for short-distance propagation in a symmetric configuration. The excellent agreement of such a solution with the result that we obtain using our perturbatively-motivated Variational Approach is then used to justify an analytical approximation that can be applied in a more general case. This allows us to find the most promising configuration for the search of photon-photon scattering in optics experiments. In particular, we show that our previous requirement of phase coherence between the two crossing beams can be released. We then propose a very simple experiment that can be performed at future exawatt laser facilities, such as ELI, by bombarding a low power laser beam with the exawatt bump.Comment: 8 pages, 6 figure

    Vortex Origin of Tricritical Point in Ginzburg-Landau Theory

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    Motivated by recent experimental progress in the critical regime of high-TcT_c superconductors we show how the tricritical point in a superconductor can be derived from the Ginzburg-Landau theory as a consequence of vortex fluctuations. Our derivation explains why usual renormalization group arguments always produce a first-order transition, in contrast to experimental evidence and Monte Carlo simulations.Comment: 4 pages,1 figur

    Single Leptoquark Production at e+ee^+e^- and γγ\gamma\gamma Colliders

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    We consider single production of leptoquarks (LQ's) at e+ee^+e^- and γγ\gamma\gamma colliders, for two values of the centre-of-mass energy, s=500\sqrt{s}=500 GeV and 1 TeV. We find that LQ's which couple within the first generation are observable for LQ masses almost up to the kinematic limit, both at e+ee^+e^- and γγ\gamma\gamma colliders, for the LQ coupling strength equal to αem\alpha_{em}. The cross sections for single production of 2nd2^{nd}- and 3rd3^{rd}-generation LQ's at e+ee^+e^- colliders are too small to be observable. In γγ\gamma\gamma collisions, on the other hand, 2nd2^{nd}-generation LQ's with masses much larger than s/2\sqrt{s}/2 can be detected. However, 3rd3^{rd}-generation LQ's can be seen at γγ\gamma\gamma colliders only for masses at most s/2\sim\sqrt{s}/2, making their observation more probable via the pair production mechanism.Comment: plain TeX, 14 pages, 6 figures (not included but available on request), some minor changes to the text, one reference added, figures and conclusions unchanged, UdeM-LPN-TH-93-152, McGill-93/2
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