4,655 research outputs found

    The geometric Cauchy problem for developable submanifolds

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    Given a smooth distribution D\mathscr{D} of mm-dimensional planes along a smooth regular curve γ\gamma in Rm+n\mathbb{R}^{m+n}, we consider the following problem: To find an mm-dimensional developable submanifold of Rm+n\mathbb{R}^{m+n}, that is, a ruled submanifold with constant tangent space along the rulings, such that its tangent bundle along γ\gamma coincides with D\mathscr{D}. In particular, we give sufficient conditions for the local well-posedness of the problem, together with a parametric description of the solution.Comment: 15 page

    TCP: exercises

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    A scattering approach to some aspects of the Schwarzschild Black Hole

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    In this paper, we consider a massless field, with spin j, in interaction with a Schwarzschild black hole in four dimensions, focusing mainly our study on the s-wave scattering. First, using a Fourier analysis, we show that one can have a simple and natural description of the Physics near the event horizon without using any conformal field approaches. Then, within the same "scattering picture", we derive analytically the imaginary part of the highly damped quasinormal complex frequencies and, as a natural consequence of our analysis, we show that thermal effects and in particular Hawking radiation, can be understood through the scattering of an ingoing s-wave by the non null barrier of the Regge-Wheeler potential associated with the Schwarzschild black hole. Finally, with the help of the well-known expression of the highly damped quasinormal complex frequencies, we propose a heuristic extension of the "tripled Pauli statistics" suggested by Motl, some years ago.Comment: 18 pages, 1 figure, JHEP accepted articl

    Cartan Ribbonization of Surfaces and a Topological Inspection

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    We develop the concept of Cartan ribbons and a method by which they can be used to ribbonize any given surface in space by intrinsically flat ribbons. The geodesic curvature along the center curve on the surface agrees with the geodesic curvature of the corresponding Cartan development curve, and this makes a rolling strategy successful. Essentially, it follows from the orientational alignment of the two co-moving Darboux frames during the rolling. Using closed center curves we obtain closed approximating Cartan ribbons that contribute zero to the total curvature integral of the ribbonization. This paves the way for a particular simple topological inspection -- it is reduced to the question of how the ribbons organize their edges relative to each other. The Gauss-Bonnet theorem leads to this topological inspection of the vertices. Finally, we display two examples of ribbonizations of surfaces, namely of a torus using two ribbons, and of an ellipsoid using its closed curvature lines as center curves for the ribbons. The topological inspection of the torus ribbonization is particularly simple as it has no vertex points, giving directly the Euler characteristic 00. The ellipsoid has 44 vertices -- corresponding to the 44 umbilical points -- each of degree one and each therefore contributing one-half to the Euler characteristic

    Fine structure of high-energy absorption cross sections for black holes

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    The high-energy absorption cross section of the Schwarzschild black hole is well approximated, in the eikonal regime, by the sum of two terms: the geometrical cross section of the black hole photon sphere and the contribution of a sinc function involving the geometrical characteristics (orbital period and Lyapunov exponent) of the null unstable geodesics lying on this photon sphere. From a numerical analysis, we show that, beyond the eikonal description, this absorption cross section presents a simple fine structure. We then describe it analytically by using Regge pole techniques and interpret it in geometrical terms. We naturally extend our analysis to arbitrary static spherically symmetric black holes endowed with a photon sphere and we then apply our formalism to Schwarzschild-Tangherlini and Reissner-Nordstr\"om black holes. Finally, on the example of the Schwarzschild black hole, we show numerically that a complicated hyperfine structure lying beyond the fine structure can also be observed.Comment: v2: Minor corrections; v3: Minor changes to match the published versio

    Marshall on Custom and Competition

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    Entry for the Elgar Companion to Alfred Marshall, edited by Tiziano Raffaelli, Marco Dardi, and Giacomo Becatini, Cheltenham: Edward Elgar 200
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