40,286 research outputs found

    Theoretical status of epsilon'/epsilon

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    The Standard Model prediction for epsilon'/epsilon is updated, taking into account the most recent theoretical developments. The final numerical value, epsilon'/\epsilon = (17\pm 6) x 10^{-4}, is in good agreement with present measurements.Comment: 6 pages. Invited talk at the 4th Int. Conference on Hyperons, Charm and Beauty Hadrons (Valencia, June 2000

    Numerical methods for multiscale inverse problems

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    We consider the inverse problem of determining the highly oscillatory coefficient aϵa^\epsilon in partial differential equations of the form (aϵuϵ)+buϵ=f-\nabla\cdot (a^\epsilon\nabla u^\epsilon)+bu^\epsilon = f from given measurements of the solutions. Here, ϵ\epsilon indicates the smallest characteristic wavelength in the problem (0<ϵ10<\epsilon\ll1). In addition to the general difficulty of finding an inverse, the oscillatory nature of the forward problem creates an additional challenge of multiscale modeling, which is hard even for forward computations. The inverse problem in its full generality is typically ill-posed and one common approach is to replace the original problem with an effective parameter estimation problem. We will here include microscale features directly in the inverse problem and avoid ill-posedness by assuming that the microscale can be accurately represented by a low-dimensional parametrization. The basis for our inversion will be a coupling of the parametrization to analytic homogenization or a coupling to efficient multiscale numerical methods when analytic homogenization is not available. We will analyze the reduced problem, b=0b = 0, by proving uniqueness of the inverse in certain problem classes and by numerical examples and also include numerical model examples for medical imaging, b>0b > 0, and exploration seismology, b<0b < 0

    Bootstrapping the Minimal 3D SCFT

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    We study the conformal bootstrap constraints for 3D conformal field theories with a Z2\mathbb{Z}_2 or parity symmetry, assuming a single relevant scalar operator ϵ\epsilon that is invariant under the symmetry. When there is additionally a single relevant odd scalar σ\sigma, we map out the allowed space of dimensions and three-point couplings of such "Ising-like" CFTs. If we allow a second relevant odd scalar σ\sigma', we identify a feature in the allowed space compatible with 3D N=1\mathcal{N}=1 superconformal symmetry and conjecture that it corresponds to the minimal N=1\mathcal{N}=1 supersymmetric extension of the Ising CFT. This model has appeared in previous numerical bootstrap studies, as well as in proposals for emergent supersymmetry on the boundaries of topological phases of matter. Adding further constraints from 3D N=1\mathcal{N}=1 superconformal symmetry, we isolate this theory and use the numerical bootstrap to compute the leading scaling dimensions Δσ=Δϵ1=.58444(22)\Delta_{\sigma} = \Delta_{\epsilon} - 1 = .58444(22) and three-point couplings λσσϵ=1.0721(2)\lambda_{\sigma\sigma\epsilon} = 1.0721(2) and λϵϵϵ=1.67(1)\lambda_{\epsilon\epsilon\epsilon} = 1.67(1). We additionally place bounds on the central charge and use the extremal functional method to estimate the dimensions of the next several operators in the spectrum. Based on our results we observe the possible exact relation λϵϵϵ/λσσϵ=tan(1)\lambda_{\epsilon\epsilon\epsilon}/\lambda_{\sigma\sigma\epsilon} = \tan(1).Comment: 16 pages, 6 figures; V2: references adde

    Test of renormalization predictions for universal finite-size scaling functions

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    We calculate universal finite-size scaling functions for systems with an n-component order parameter and algebraically decaying interactions. Just as previously has been found for short-range interactions, this leads to a singular epsilon-expansion, where epsilon is the distance to the upper critical dimension. Subsequently, we check the results by numerical simulations of spin models in the same universality class. Our systems offer the essential advantage that epsilon can be varied continuously, allowing an accurate examination of the region where epsilon is small. The numerical calculations turn out to be in striking disagreement with the predicted singularity.Comment: 6 pages, including 3 EPS figures. To appear in Phys. Rev. E. Also available as PDF file at http://www.cond-mat.physik.uni-mainz.de/~luijten/erikpubs.htm
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