50,877 research outputs found

    Effects of Scale-Free Disorder on the Anderson Metal-Insulator Transition

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    We investigate the three-dimensional Anderson model of localization via a modified transfer-matrix method in the presence of scale-free diagonal disorder characterized by a disorder correlation function g(r)g(r) decaying asymptotically as rαr^{-\alpha}. We study the dependence of the localization-length exponent ν\nu on the correlation-strength exponent α\alpha. % For fixed disorder WW, there is a critical αc\alpha_{\rm c}, such that for α<αc\alpha < \alpha_{\rm c}, ν=2/α\nu=2/\alpha and for α>αc\alpha > \alpha_{\rm c}, ν\nu remains that of the uncorrelated system in accordance with the extended Harris criterion. At the band center, ν\nu is independent of α\alpha but equal to that of the uncorrelated system. The physical mechanisms leading to this different behavior are discussed.Comment: submitted to Phys. Rev. Let

    Critical Behaviour of 3D Systems with Long-Range Correlated Quenched Defects

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    A field-theoretic description of the critical behaviour of systems with quenched defects obeying a power law correlations xa\sim |{\bf x}|^{-a} for large separations x{\bf x} is given. Directly for three-dimensional systems and different values of correlation parameter 2a32\leq a \leq 3 a renormalization analysis of scaling function in the two-loop approximation is carried out, and the fixed points corresponding to stability of the various types of critical behaviour are identified. The obtained results essentially differ from results evaluated by double ϵ,δ\epsilon, \delta - expansion. The critical exponents in the two-loop approximation are calculated with the use of the Pade-Borel summation technique.Comment: Submitted to J. Phys. A, Letter to Editor 9 pages, 4 figure

    The Causal Boundary of spacetimes revisited

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    We present a new development of the causal boundary of spacetimes, originally introduced by Geroch, Kronheimer and Penrose. Given a strongly causal spacetime (or, more generally, a chronological set), we reconsider the GKP ideas to construct a family of completions with a chronology and topology extending the original ones. Many of these completions present undesirable features, like those appeared in previous approaches by other authors. However, we show that all these deficiencies are due to the attachment of an ``excessively big'' boundary. In fact, a notion of ``completion with minimal boundary'' is then introduced in our family such that, when we restrict to these minimal completions, which always exist, all previous objections disappear. The optimal character of our construction is illustrated by a number of satisfactory properties and examples.Comment: 37 pages, 10 figures; Definition 6.1 slightly modified; multiple minor changes; one figure added and another replace

    Storage of light in atomic vapor

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    We report an experiment in which a light pulse is decelerated and trapped in a vapor of Rb atoms, stored for a controlled period of time, and then released on demand. We accomplish this storage of light by dynamically reducing the group velocity of the light pulse to zero, so that the coherent excitation of the light is reversibly mapped into a collective Zeeman (spin) coherence of the Rb vapor

    Spin ice in a field: quasi-phases and pseudo-transitions

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    Thermodynamics of the short-range model of spin ice magnets in a field is considered in the Bethe - Peierls approximation. The results obtained for [111], [100] and [011] fields agrees reasonably well with the existing Monte-Carlo simulations and some experiments. In this approximation all extremely sharp field-induced anomalies are described by the analytical functions of temperature and applied field. In spite of the absence of true phase transitions the analysis of the entropy and specific heat reliefs over H-T plane allows to discern the "pseudo-phases" with specific character of spin fluctuations and define the lines of more or less sharp "pseudo-transitions" between them.Comment: 18 pages, 16 figure

    Slow group velocity and Cherenkov radiation

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    We theoretically study the effect of ultraslow group velocities on the emission of Vavilov-Cherenkov radiation in a coherently driven medium. We show that in this case the aperture of the group cone on which the intensity of the radiation peaks is much smaller than that of the usual wave cone associated with the Cherenkov coherence condition. We show that such a singular behaviour may be observed in a coherently driven ultracold atomic gas.Comment: 4 pages, 4 figure

    PTF11kx: A Type Ia Supernova with Hydrogen Emission Persisting After 3.5 Years

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    The optical transient PTF11kx exhibited both the characteristic spectral features of Type Ia supernovae (SNe Ia) and the signature of ejecta interacting with circumstellar material (CSM) containing hydrogen, indicating the presence of a nondegenerate companion. We present an optical spectrum at 13421342 days after peak from Keck Observatory, in which the broad component of Hα\alpha emission persists with a similar profile as in early-time observations. We also present SpitzerSpitzer IRAC detections obtained 12371237 and 18181818 days after peak, and an upper limit from HSTHST ultraviolet imaging at 21332133 days. We interpret our late-time observations in context with published results - and reinterpret the early-time observations - in order to constrain the CSM's physical parameters and compare to theoretical predictions for recurrent nova systems. We find that the CSM's radial extent may be several times the distance between the star and the CSM's inner edge, and that the CSM column density may be two orders of magnitude lower than previous estimates. We show that the Hα\alpha luminosity decline is similar to other SNe with CSM interaction, and demonstrate how our infrared photometry is evidence for newly formed, collisionally heated dust. We create a model for PTF11kx's late-time CSM interaction and find that X-ray reprocessing by photoionization and recombination cannot reproduce the observed Hα\alpha luminosity, suggesting that the X-rays are thermalized and that Hα\alpha radiates from collisional excitation. Finally, we discuss the implications of our results regarding the progenitor scenario and the geometric properties of the CSM for the PTF11kx system.Comment: 15 pages, 8 figures, 3 tables; submitted to Ap
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