4,638 research outputs found

    Turan's method and compressive sampling

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    Turan's method, as expressed in his books, is a careful study of trigonometric polynomials from different points of view. The present article starts from a problem asked by Turan: how to construct a sequence of real numbers x(j) (j= 1,2,...n) such that the almost periodic polynomial whose frequencies are the x(j) and the coefficients are 1 are small (say, their absolute values are less than n d, d< given) for all integral values of the variable m between 1 and M= M(n,d) ? The best known answer is a random choice of the x(j) modulo 1. Using the random choice as Turan (and before him Erd\"os and Renyi), we improve the estimate of M (n, d) and we discuss an explicit construction derived from another chapter of Turan's book. The main part of the paper deals with the corresponding problem when R / Z is replaced by Z / NZ, N prime, and m takes all integral values modulo 1 except 0. Then it has an interpretation in signal theory, when a signal is representad by a function on the cyclic goup G = Z / NZ and the frequencies by the dual cyclic group G^ : knowing that the signal is carried by T points, to evaluate the probability that a random choice of a set W of frequencies allows to recover the signal x from the restriction of its Fourier tranform to W by the process of minimal extrapolation in the Wiener algebra of G^(process of Cand\`es, Romberg and Tao). Some random choices were considered in the original article of CRT and the corresponding probabilities were estimated in two preceding papers of mine. Here we have another random choice, associated with occupancy problems

    Italo-Byzantine etymologies IV

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    On uniform convergence of Fourier series

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    We consider the space U(T)U(\mathbb T) of all continuous functions on the circle T\mathbb T with uniformly convergent Fourier series. We show that if φ:TT\varphi: \mathbb T\rightarrow\mathbb T is a continuous piecewise linear but not linear map, then einφU(T)logn\|e^{in\varphi}\|_{U(\mathbb T)}\simeq\log n

    Packing-Dimension Profiles and Fractional Brownian Motion

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    In order to compute the packing dimension of orthogonal projections Falconer and Howroyd (1997) introduced a family of packing dimension profiles Dims{\rm Dim}_s that are parametrized by real numbers s>0s>0. Subsequently, Howroyd (2001) introduced alternate ss-dimensional packing dimension profiles \hbox{{\rm P}-\dim}_s and proved, among many other things, that \hbox{{\rm P}-\dim}_s E={\rm Dim}_s E for all integers s>0s>0 and all analytic sets ERNE\subseteq\R^N. The goal of this article is to prove that \hbox{{\rm P}-\dim}_s E={\rm Dim}_s E for all real numbers s>0s>0 and analytic sets ERNE\subseteq\R^N. This answers a question of Howroyd (2001, p. 159). Our proof hinges on a new property of fractional Brownian motion

    Enhancement and Civic Virtue

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    Opponents of biomedical enhancement frequently adopt what Allen Buchanan has called the “Personal Goods Assumption.” On this assumption, the benefits of biomedical enhancement will accrue primarily to those individuals who undergo enhancements, not to wider society. Buchanan has argued that biomedical enhancements might in fact have substantial social benefits by increasing productivity. We outline another way in which enhancements might benefit wider society: by augmenting civic virtue and thus improving the functioning of our political communities. We thus directly confront critics of biomedical enhancement who argue that it will lead to a loss of social cohesion and a breakdown in political lif

    The census of complex organic molecules in the solar type protostar IRAS16293-2422

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    Complex Organic Molecules (COMs) are considered crucial molecules, since they are connected with organic chemistry, at the basis of the terrestrial life. More pragmatically, they are molecules in principle difficult to synthetize in the harsh interstellar environments and, therefore, a crucial test for astrochemical models. Current models assume that several COMs are synthesised on the lukewarm grain surfaces (\gtrsim30-40 K), and released in the gas phase at dust temperatures \gtrsim100 K. However, recent detections of COMs in \lesssim20 K gas demonstrate that we still need important pieces to complete the puzzle of the COMs formation. We present here a complete census of the oxygen and nitrogen bearing COMs, previously detected in different ISM regions, towards the solar type protostar IRAS16293-2422. The census was obtained from the millimeter-submillimeter unbiased spectral survey TIMASSS. Six COMs, out of the 29 searched for, were detected: methyl cyanide, ketene, acetaldehyde, formamide, dimethyl ether, and methyl formate. The multifrequency analysis of the last five COMs provides clear evidence that they are present in the cold (\lesssim30 K) envelope of IRAS16293-2422, with abundances 0.03-2 ×1010\times 10^{-10}. Our data do not allow to support the hypothesis that the COMs abundance increases with increasing dust temperature in the cold envelope, as expected if COMs were predominately formed on the lukewarm grain surfaces. Finally, when considering also other ISM sources, we find a strong correlation over five orders of magnitude, between the methyl formate and dimethyl ether and methyl formate and formamide abundances, which may point to a link between these two couples of species, in cold and warm gas
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