4,410,261 research outputs found

    Local Whittle estimation in nonstationary and unit root cases

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    Asymptotic properties of the local Whittle estimator in the nonstationary case (d>{1/2}) are explored. For {1/2}<d\leq 1, the estimator is shown to be consistent, and its limit distribution and the rate of convergence depend on the value of d. For d=1, the limit distribution is mixed normal. For d>1 and when the process has a polynomial trend of order \alpha >{1/2}, the estimator is shown to be inconsistent and to converge in probability to unity

    Quantum Gravity in Large Dimensions

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    Quantum gravity is investigated in the limit of a large number of space-time dimensions, using as an ultraviolet regularization the simplicial lattice path integral formulation. In the weak field limit the appropriate expansion parameter is determined to be 1/d1/d. For the case of a simplicial lattice dual to a hypercube, the critical point is found at kc/λ=1/dk_c/\lambda=1/d (with k=1/8πGk=1/8 \pi G) separating a weak coupling from a strong coupling phase, and with 2d22 d^2 degenerate zero modes at kck_c. The strong coupling, large GG, phase is then investigated by analyzing the general structure of the strong coupling expansion in the large dd limit. Dominant contributions to the curvature correlation functions are described by large closed random polygonal surfaces, for which excluded volume effects can be neglected at large dd, and whose geometry we argue can be approximated by unconstrained random surfaces in this limit. In large dimensions the gravitational correlation length is then found to behave as log(kck)1/2| \log (k_c - k) |^{1/2}, implying for the universal gravitational critical exponent the value ν=0\nu=0 at d=d=\infty.Comment: 47 pages, 2 figure

    2-d Gravity as a Limit of the SL(2,R) Black Hole

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    The transformation of the SL(2,R)/U(1)SL(2,R)/U(1) black hole under a boost of the subgroup U(1) is studied. It is found that the tachyon vertex operators of the black hole go into those of the c=1c=1 conformal field theory coupled to gravity. The discrete states of the black hole also tend to the discrete states of the 2-d gravity theory. The fate of the extra discrete states of the black hole under boost are discussed.Comment: LaTeX file, 14 page

    Renormalization Group Approach to Interacting Crumpled Surfaces: The hierarchical recursion

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    We study the scaling limit of a model of a tethered crumpled D-dimensional random surface interacting through an exclusion condition with a fixed impurity in d-dimensional Euclidean space by the methods of Wilson's renormalization group. In this paper we consider a hierarchical version of the model and we prove rigorously the existence of the scaling limit and convergence to a non-Gaussian fixed point for 1D01 \leq D0 sufficiently small, where ϵ=D(2D)d2\epsilon = D - (2-D) {d\over 2}.Comment: 47 pages in simple Latex, PAR-LPTHE 934

    Random Sequential Addition of Hard Spheres in High Euclidean Dimensions

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    Employing numerical and theoretical methods, we investigate the structural characteristics of random sequential addition (RSA) of congruent spheres in dd-dimensional Euclidean space Rd\mathbb{R}^d in the infinite-time or saturation limit for the first six space dimensions (1d61 \le d \le 6). Specifically, we determine the saturation density, pair correlation function, cumulative coordination number and the structure factor in each =of these dimensions. We find that for 2d62 \le d \le 6, the saturation density ϕs\phi_s scales with dimension as ϕs=c1/2d+c2d/2d\phi_s= c_1/2^d+c_2 d/2^d, where c1=0.202048c_1=0.202048 and c2=0.973872c_2=0.973872. We also show analytically that the same density scaling persists in the high-dimensional limit, albeit with different coefficients. A byproduct of this high-dimensional analysis is a relatively sharp lower bound on the saturation density for any dd given by ϕs(d+2)(1S0)/2d+1\phi_s \ge (d+2)(1-S_0)/2^{d+1}, where S0[0,1]S_0\in [0,1] is the structure factor at k=0k=0 (i.e., infinite-wavelength number variance) in the high-dimensional limit. Consistent with the recent "decorrelation principle," we find that pair correlations markedly diminish as the space dimension increases up to six. Our work has implications for the possible existence of disordered classical ground states for some continuous potentials in sufficiently high dimensions.Comment: 38 pages, 9 figures, 4 table

    Continuum limit of string formation in 3-d SU(2) LGT

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    We study the continuum limit of the string-like behaviour of flux tubes formed between static quarks and anti-quarks in three dimensional SU(2) lattice gauge theory. We compare our simulation data with the predictions of both effective string models as well as perturbation theory. On the string side we obtain clear evidence for convergence of data to predictions of Nambu-Goto theory. We comment on the scales at which the static potential starts departing from one loop perturbation theory and then again being well described by effective string theories. We also estimate the leading corrections to the one-loop perturbative potential as well as the Nambu-Goto effective string. In the intermediate regions we find that a modified Lennard-Jones type potential gives surprisingly good fits.Comment: 13 pages, 3 figures and 6 table

    Stochastic heat equation limit of a (2+1)d growth model

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    We determine a q1q\to 1 limit of the two-dimensional qq-Whittaker driven particle system on the torus studied previously in [Corwin-Toninelli, arXiv:1509.01605]. This has an interpretation as a (2+1)(2+1)-dimensional stochastic interface growth model, that is believed to belong to the so-called anisotropic Kardar-Parisi-Zhang (KPZ) class. This limit falls into a general class of two-dimensional systems of driven linear SDEs which have stationary measures on gradients. Taking the number of particles to infinity we demonstrate Gaussian free field type fluctuations for the stationary measure. Considering the temporal evolution of the stationary measure, we determine that along characteristics, correlations are asymptotically given by those of the (2+1)(2+1)-dimensional additive stochastic heat equation. This confirms (for this model) the prediction that the non-linearity for the anisotropic KPZ equation in (2+1)(2+1)-dimension is irrelevant.Comment: 24 pages, 1 figur
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