1,608 research outputs found

    Density of States of Quantum Spin Systems from Isotropic Entanglement

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    We propose a method which we call "Isotropic Entanglement" (IE), that predicts the eigenvalue distribution of quantum many body (spin) systems (QMBS) with generic interactions. We interpolate between two known approximations by matching fourth moments. Though, such problems can be QMA-complete, our examples show that IE provides an accurate picture of the spectra well beyond what one expects from the first four moments alone. We further show that the interpolation is universal, i.e., independent of the choice of local terms.Comment: 4+ pages, content is as in the published versio

    Systematics of Aligned Axions

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    We describe a novel technique that renders theories of NN axions tractable, and more generally can be used to efficiently analyze a large class of periodic potentials of arbitrary dimension. Such potentials are complex energy landscapes with a number of local minima that scales as N!\sqrt{N!}, and so for large NN appear to be analytically and numerically intractable. Our method is based on uncovering a set of approximate symmetries that exist in addition to the NN periods. These approximate symmetries, which are exponentially close to exact, allow us to locate the minima very efficiently and accurately and to analyze other characteristics of the potential. We apply our framework to evaluate the diameters of flat regions suitable for slow-roll inflation, which unifies, corrects and extends several forms of "axion alignment" previously observed in the literature. We find that in a broad class of random theories, the potential is smooth over diameters enhanced by N3/2N^{3/2} compared to the typical scale of the potential. A Mathematica implementation of our framework is available online.Comment: 68 pages, 17 figure

    Approximate null distribution of the largest root in multivariate analysis

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    The greatest root distribution occurs everywhere in classical multivariate analysis, but even under the null hypothesis the exact distribution has required extensive tables or special purpose software. We describe a simple approximation, based on the Tracy--Widom distribution, that in many cases can be used instead of tables or software, at least for initial screening. The quality of approximation is studied, and its use illustrated in a variety of setttings.Comment: Published in at http://dx.doi.org/10.1214/08-AOAS220 the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org

    Superstatistical generalisations of Wishart-Laguerre ensembles of random matrices

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    Using Beck and Cohen's superstatistics, we introduce in a systematic way a family of generalized Wishart–Laguerre ensembles of random matrices with Dyson index β = 1, 2 and 4. The entries of the data matrix are Gaussian random variables whose variances η fluctuate from one sample to another according to a certain probability density f(η) and a single deformation parameter γ. Three superstatistical classes for f(η) are usually considered: χ2-, inverse χ2- and log-normal distributions. While the first class, already considered by two of the authors, leads to a power-law decay of the spectral density, we here introduce and solve exactly a superposition of Wishart–Laguerre ensembles with inverse χ2-distribution. The corresponding macroscopic spectral density is given by a γ-deformation of the semi-circle and Marčenko–Pastur laws, on a non-compact support with exponential tails. After discussing in detail the validity of Wigner's surmise in the Wishart–Laguerre class, we introduce a generalized γ-dependent surmise with stretched-exponential tails, which well approximates the individual level spacing distribution in the bulk. The analytical results are in excellent agreement with numerical simulations. To illustrate our findings we compare the χ2- and inverse χ2-classes to empirical data from financial covariance matrices

    Planckian Axions in String Theory

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    We argue that super-Planckian diameters of axion fundamental domains can naturally arise in Calabi-Yau compactifications of string theory. In a theory with NN axions θi\theta^i, the fundamental domain is a polytope defined by the periodicities of the axions, via constraints of the form −π<Qjiθj<π-\pi<Q^{i}_{j} \theta^j<\pi. We compute the diameter of the fundamental domain in terms of the eigenvalues f12≤.˙.≤fN2f_1^2\le\...\le f_N^2 of the metric on field space, and also, crucially, the largest eigenvalue of (QQ⊤)−1(QQ^{\top})^{-1}. At large NN, QQ⊤QQ^{\top} approaches a Wishart matrix, due to universality, and we show that the diameter is at least NfNN f_{N}, exceeding the naive Pythagorean range by a factor >N>\sqrt{N}. This result is robust in the presence of P>NP>N constraints, while for P=NP=N the diameter is further enhanced by eigenvector delocalization to N3/2fNN^{3/2}f_N. We directly verify our results in explicit Calabi-Yau compactifications of type IIB string theory. In the classic example with h1,1=51h^{1,1}=51 where parametrically controlled moduli stabilization was demonstrated by Denef et al. in [1], the largest metric eigenvalue obeys fN≈0.013Mplf_N \approx 0.013 M_{pl}. The random matrix analysis then predicts, and we exhibit, axion diameters >Mpl>M_{pl} for the precise vacuum parameters found in [1]. Our results provide a framework for achieving large-field axion inflation in well-understood flux vacua.Comment: 42 pages, 4 figure
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