1,849 research outputs found

    A New Duality Between N=8\mathcal{N}=8 Superconformal Field Theories in Three Dimensions

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    We propose a new duality between two 3d N=8\mathcal{N}=8 superconformal Chern-Simons-matter theories: the U(3)1×U(3)1U(3)_1 \times U(3)_{-1} ABJM theory and a theory consisting of the product between the (SU(2)3×SU(2)3)/Z2\left(SU(2)_3\times SU(2)_{-3}\right)/\mathbb{Z}_2 BLG theory and a free N=8{\cal N} = 8 theory of eight real scalars and eight Majorana fermions. As evidence supporting this duality, we show that the moduli spaces, superconformal indices, S3S^3 partition functions, and certain OPE coefficients of BPS operators in the two theories agree.Comment: 29 pages, 2 figure

    Solving M-theory with the Conformal Bootstrap

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    We use the conformal bootstrap to perform a precision study of 3d maximally supersymmetric (N=8\mathcal{N}=8) SCFTs that describe the IR physics on NN coincident M2-branes placed either in flat space or at a \C^4/\Z_2 singularity. First, using the explicit Lagrangians of ABJ(M) \cite{Aharony:2008ug,Aharony:2008gk} and recent supersymmetric localization results, we calculate certain half and quarter-BPS OPE coefficients, both exactly at small NN, and approximately in a large NN expansion that we perform to all orders in 1/N1/N. Comparing these values with the numerical bootstrap bounds leads us to conjecture that some of these theories obey an OPE coefficient minimization principle. We then use this conjecture as well as the extremal functional method to reconstruct the first few low-lying scaling dimensions and OPE coefficients for both protected and unprotected multiplets that appear in the OPE of two stress tensor multiplets for all values of NN. We also calculate the half and quarter-BPS operator OPE coefficients in the SU(2)k×SU(2)kSU(2)_k \times SU(2)_{-k} BLG theory for all values of the Chern-Simons coupling kk, and show that generically they do not obey the same OPE coefficient minimization principle.Comment: 30 pages, 5 figures, v2 submitted for publicatio

    Emergence of Periodic Structure from Maximizing the Lifetime of a Bound State Coupled to Radiation

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    Consider a system governed by the time-dependent Schr\"odinger equation in its ground state. When subjected to weak (size ϵ\epsilon) parametric forcing by an "ionizing field" (time-varying), the state decays with advancing time due to coupling of the bound state to radiation modes. The decay-rate of this metastable state is governed by {\it Fermi's Golden Rule}, Γ[V]\Gamma[V], which depends on the potential VV and the details of the forcing. We pose the potential design problem: find VoptV_{opt} which minimizes Γ[V]\Gamma[V] (maximizes the lifetime of the state) over an admissible class of potentials with fixed spatial support. We formulate this problem as a constrained optimization problem and prove that an admissible optimal solution exists. Then, using quasi-Newton methods, we compute locally optimal potentials. These have the structure of a truncated periodic potential with a localized defect. In contrast to optimal structures for other spectral optimization problems, our optimizing potentials appear to be interior points of the constraint set and to be smooth. The multi-scale structures that emerge incorporate the physical mechanisms of energy confinement via material contrast and interference effects. An analysis of locally optimal potentials reveals local optimality is attained via two mechanisms: (i) decreasing the density of states near a resonant frequency in the continuum and (ii) tuning the oscillations of extended states to make Γ[V]\Gamma[V], an oscillatory integral, small. Our approach achieves lifetimes, (ϵ2Γ[V])1\sim (\epsilon^2\Gamma[V])^{-1}, for locally optimal potentials with Γ1O(109)\Gamma^{-1}\sim\mathcal{O}(10^{9}) as compared with Γ1O(102)\Gamma^{-1}\sim \mathcal{O}(10^{2}) for a typical potential. Finally, we explore the performance of optimal potentials via simulations of the time-evolution.Comment: 33 pages, 6 figure

    Gravitational waves in general relativity: XIV. Bondi expansions and the ``polyhomogeneity'' of \Scri

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    The structure of polyhomogeneous space-times (i.e., space-times with metrics which admit an expansion in terms of rjlogirr^{-j}\log^i r) constructed by a Bondi--Sachs type method is analysed. The occurrence of some log terms in an asymptotic expansion of the metric is related to the non--vanishing of the Weyl tensor at Scri. Various quantities of interest, including the Bondi mass loss formula, the peeling--off of the Riemann tensor and the Newman--Penrose constants of motion are re-examined in this context.Comment: LaTeX, 28pp, CMA-MR14-9

    Sharp spectral stability estimates via the Lebesgue measure of domains for higher order elliptic operators

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    We prove sharp stability estimates for the variation of the eigenvalues of non-negative self-adjoint elliptic operators of arbitrary even order upon variation of the open sets on which they are defined. These estimates are expressed in terms of the Lebesgue measure of the symmetric difference of the open sets. Both Dirichlet and Neumann boundary conditions are considered

    On thin plate spline interpolation

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    We present a simple, PDE-based proof of the result [M. Johnson, 2001] that the error estimates of [J. Duchon, 1978] for thin plate spline interpolation can be improved by h1/2h^{1/2}. We illustrate that H{\mathcal H}-matrix techniques can successfully be employed to solve very large thin plate spline interpolation problem

    Eigenfunctions decay for magnetic pseudodifferential operators

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    We prove rapid decay (even exponential decay under some stronger assumptions) of the eigenfunctions associated to discrete eigenvalues, for a class of self-adjoint operators in L2(Rd)L^2(\mathbb{R}^d) defined by ``magnetic'' pseudodifferential operators (studied in \cite{IMP1}). This class contains the relativistic Schr\"{o}dinger operator with magnetic field

    Motion of Isolated bodies

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    It is shown that sufficiently smooth initial data for the Einstein-dust or the Einstein-Maxwell-dust equations with non-negative density of compact support develop into solutions representing isolated bodies in the sense that the matter field has spatially compact support and is embedded in an exterior vacuum solution

    Hardy-Carleman Type Inequalities for Dirac Operators

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    General Hardy-Carleman type inequalities for Dirac operators are proved. New inequalities are derived involving particular traditionally used weight functions. In particular, a version of the Agmon inequality and Treve type inequalities are established. The case of a Dirac particle in a (potential) magnetic field is also considered. The methods used are direct and based on quadratic form techniques
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