928 research outputs found

    Juhl's Formulae for GJMS Operators and Q-Curvatures

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    Direct proofs are given of Juhl's formulae for GJMS operators and Q-curvatures starting from the original construction of GJMS.Comment: 18 page

    Entanglement entropy of black holes and AdS/CFT correspondence

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    A recent proposal by Ryu and Takayanagi for a holographic interpretation of entanglement entropy in conformal field theories dual to supergravity on anti-de Sitter (adS) is generalized to include entanglement entropy of black holes living on the boundary of adS. The generalized proposal is verified in boundary dimensions d=2d=2 and d=4d=4 for both the UV divergent and UV finite terms. In dimension d=4d=4 an expansion of entanglement entropy in terms of size LL of the subsystem outside the black hole is considered. A new term in the entropy of dual strongly coupled CFT, which universally grows as L2lnLL^2\ln L and is proportional to the value of the obstruction tensor at the black hole horizon, is predicted.Comment: 5 pages; minor typos corrected, minor changes in text. Version accepted for publication in Phys. Rev. Let

    On the Whitney distortion extension problem for Cm(Rn)C^m(\mathbb R^n) and C(Rn)C^{\infty}(\mathbb R^n) and its applications to interpolation and alignment of data in Rn\mathbb R^n

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    Let n,m1n,m\geq 1, URnU\subset\mathbb R^n open. In this paper we provide a sharp solution to the following Whitney distortion extension problems: (a) Let ϕ:URn\phi:U\to \mathbb R^n be a CmC^m map. If EUE\subset U is compact (with some geometry) and the restriction of ϕ\phi to EE is an almost isometry with small distortion, how to decide when there exists a Cm(Rn)C^m(\mathbb R^n) one-to-one and onto almost isometry Φ:RnRn\Phi:\mathbb R^n\to \mathbb R^n with small distortion which agrees with ϕ\phi in a neighborhood of EE and a Euclidean motion A:RnRnA:\mathbb R^n\to \mathbb R^n away from EE. (b) Let ϕ:URn\phi:U\to \mathbb R^n be CC^{\infty} map. If EUE\subset U is compact (with some geometry) and the restriction of ϕ\phi to EE is an almost isometry with small distortion, how to decide when there exists a C(Rn)C^{\infty}(\mathbb R^n) one-to-one and onto almost isometry Φ:RnRn\Phi:\mathbb R^n\to \mathbb R^n with small distortion which agrees with ϕ\phi in a neighborhood of EE and a Euclidean motion A:RnRnA:\mathbb R^n\to \mathbb R^n away from EE. Our results complement those of [14,15,20] where there, EE is a finite set. In this case, the problem above is also a problem of interpolation and alignment of data in Rn\mathbb R^n.Comment: This is part three of four papers with C. Fefferman (arXiv:1411.2451, arXiv:1411.2468, involve-v5-n2-p03-s.pdf) dealing with the problem of Whitney type extensions of δ>0\delta>0 distortions from certain compact sets ERnE\subset \Bbb R^n to ε>0\varepsilon>0 distorted diffeomorphisms on $\Bbb R^n

    Ambient connections realising conformal Tractor holonomy

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    For a conformal manifold we introduce the notion of an ambient connection, an affine connection on an ambient manifold of the conformal manifold, possibly with torsion, and with conditions relating it to the conformal structure. The purpose of this construction is to realise the normal conformal tractor holonomy as affine holonomy of such a connection. We give an example of an ambient connection for which this is the case, and which is torsion free if we start the construction with a C-space, and in addition Ricci-flat if we start with an Einstein manifold. Thus for a CC-space this example leads to an ambient metric in the weaker sense of \v{C}ap and Gover, and for an Einstein space to a Ricci-flat ambient metric in the sense of Fefferman and Graham.Comment: 17 page

    Non-conservation of dimension in divergence-free solutions of passive and active scalar systems

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    For any h(1,2]h\in(1,2], we give an explicit construction of a compactly supported, uniformly continuous, and (weakly) divergence-free velocity field in R2\mathbb{R}^2 that weakly advects a measure whose support is initially the origin but for positive times has Hausdorff dimension hh. These velocities are uniformly continuous in space-time and compactly supported, locally Lipschitz except at one point and satisfy the conditions for the existence and uniqueness of a Regular Lagrangian Flow in the sense of Di Perna and Lions theory. We then construct active scalar systems in R2\mathbb{R}^2 and R3\mathbb{R}^3 with measure-valued solutions whose initial support has co-dimension 2 but such that at positive times it only has co-dimension 1. The associated velocities are divergence free, compactly supported, continuous, and sufficiently regular to admit unique Regular Lagrangian Flows. This is in part motivated by the investigation of dimension conservation for the support of measure-valued solutions to active scalar systems. This question occurs in the study of vortex filaments in the three-dimensional Euler equations.Comment: 32 pages, 3 figures. This preprint has not undergone peer review (when applicable) or any post-submission improvements or corrections. The Version of Record of this article is published in Arch Rational Mech Anal, and is available online at https://doi.org/10.1007/s00205-021-01708-
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