3,295 research outputs found

    Spectrum of radiation from axion strings

    Get PDF
    In the wide variety of axion cosmologies in which axion strings form, their radiative decay is the dominant mechanism for the production of axions, imposing a tight constraint on the axion mass. Here, we focus on the mechanism by which axions are produced in this scenario and, in particular, the key issue of the axion spectrum emitted by an evolving network of strings.Comment: to be published in the proceedings of the 5th IFT Workshop on Axion

    Dissipation in a 2-dimensional Hilbert space: Various forms of complete positivity

    Full text link
    We consider the time evolution of the density matrix ρ\rho in a 2-dimensional complex Hilbert space. We allow for dissipation by adding to the von Neumann equation a term D[ρ]D[\rho], which is of Lindblad type in order to assure complete positivity of the time evolution. We present five equivalent forms of D[ρ]D[\rho]. In particular, we connect the familiar dissipation matrix LL with a geometric version of D[ρ]D[\rho], where LL consists of a positive sum of projectors onto planes in R3\mathbf{R}^3. We also study the minimal number of Lindblad terms needed to describe the most general case of D[ρ]D[\rho]. All proofs are worked out comprehensively, as they present at the same time a practical procedure how to determine explicitly the different forms of D[ρ]D[\rho]. Finally, we perform a general discussion of the asymptotic behaviour tt \to \infty of the density matrix and we relate the two types of asymptotic behaviour with our geometric version of D[ρ]D[\rho].Comment: 11 pages, LaTeX, no figures. Further aspects of complete positivity worked out and references added; version accepted for publication in Phys. Lett.

    Statistics of Wave Functions in Coupled Chaotic Systems

    Full text link
    Using the supersymmetry technique, we calculate the joint distribution of local densities of electron wavefunctions in two coupled disordered or chaotic quantum billiards. We find novel spatial correlations that are absent in a single chaotic system. Our exact result can be interpreted for small coupling in terms of the hybridization of eigenstates of the isolated billiards. We show that the presented picture is universal, independent of microscopic details of the coupling.Comment: 4 pages, 2 figures; acknowledgements and references adde

    A Pair of Disjoint 3-GDDs of type g^t u^1

    Full text link
    Pairwise disjoint 3-GDDs can be used to construct some optimal constant-weight codes. We study the existence of a pair of disjoint 3-GDDs of type gtu1g^t u^1 and establish that its necessary conditions are also sufficient.Comment: Designs, Codes and Cryptography (to appear

    State sampling dependence of the Hopfield network inference

    Get PDF
    The fully connected Hopfield network is inferred based on observed magnetizations and pairwise correlations. We present the system in the glassy phase with low temperature and high memory load. We find that the inference error is very sensitive to the form of state sampling. When a single state is sampled to compute magnetizations and correlations, the inference error is almost indistinguishable irrespective of the sampled state. However, the error can be greatly reduced if the data is collected with state transitions. Our result holds for different disorder samples and accounts for the previously observed large fluctuations of inference error at low temperatures.Comment: 4 pages, 1 figure, further discussions added and relevant references adde

    Skyrmion Excitation in Two-Dimensional Spinor Bose-Einstein Condensate

    Full text link
    We study the properties of coreless vortices(skyrmion) in spinor Bose-Einstein condensate. We find that this excitation is always energetically unstable, it always decays to an uniform spin texture. We obtain the skyrmion energy as a function of its size and position, a key quantity in understanding the decay process. We also point out that the decay rate of a skyrmion with high winding number will be slower. The interaction between skyrmions and other excitation modes are also discussed.Comment: 5 pages, 4 figures, final version published in Phys. Rev.

    Weak-Localization in Chaotic Versus Non-Chaotic Cavities: A Striking Difference in the Line Shape

    Full text link
    We report experimental evidence that chaotic and non-chaotic scattering through ballistic cavities display distinct signatures in quantum transport. In the case of non-chaotic cavities, we observe a linear decrease in the average resistance with magnetic field which contrasts markedly with a Lorentzian behavior for a chaotic cavity. This difference in line-shape of the weak-localization peak is related to the differing distribution of areas enclosed by electron trajectories. In addition, periodic oscillations are observed which are probably associated with the Aharonov-Bohm effect through a periodic orbit within the cavities.Comment: 4 pages revtex + 4 figures on request; amc.hub.94.

    Massive Charged Scalar Quasinormal Modes of Reissner-N\"ordstrom Black Hole Surrounded by Quintessence

    Full text link
    We evaluate the complex frequencies of the normal modes for the massive charged scalar field perturbations around a Reissner-N\"ordstrom black hole surrounded by a static and spherically symmetric quintessence using third order WKB approximation approach. Due to the presence of quintessence, quasinormal frequencies damp more slowly. We studied the variation of quasinormal frequencies with charge of the black bole, mass and charge of perturbating scalar field and the quintessential state parameter.Comment: 9 pages, 9 figures and one tabl

    On the ratio of consecutive gaps between primes

    Get PDF
    In the present work we prove a common generalization of Maynard-Tao's recent result about consecutive bounded gaps between primes and on the Erd\H{o}s-Rankin bound about large gaps between consecutive primes. The work answers in a strong form a 60 years old problem of Erd\"os, which asked whether the ratio of two consecutive primegaps can be infinitely often arbitrarily small, and arbitrarily large, respectively
    corecore