17,872 research outputs found

    Areal interpolation and the UK’s referendum on EU membership

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    I show how results from the United Kingdom’s referendum on membership of the European Union can be remapped from local authority level to parliamentary constituency level through the use of a scaled Poisson regression model which incorporates demographic information from lower level geographies. I use these estimates to show how the geographic distribution of signatures to a petition for a second referendum was strongly associated with how constituencies voted in the actual referendum

    Abelian Landau-Pomeranchuk-Migdal effects

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    It is shown that the high-energy expansion of the scattering amplitude calculated from Feynman diagrams factorizes in such a way that it can be reduced to the eikonalized form up to the terms of inverse power in energy in accordance with results obtained by solving the Klein-Gordon equation. Therefore the two approaches when applied to the suppression of the emission of soft photons by fast charged particles in dense matter should give rise to the same results. A particular limit of thin targets is briefly discussed.Comment: 14 pages, LATEX, 1 Fig. ps, submitted to Mod. Phys. Lett.

    Multiple Reggeon Exchange from Summing QCD Feynman Diagrams

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    Multiple reggeon exchange supplies subleading logs that may be used to restore unitarity to the Low-Nussinov Pomeron, provided it can be proven that the sum of Feynman diagrams to all orders gives rise to such multiple regge exchanges. This question cannot be easily tackled in the usual way except for very low-order diagrams, on account of delicate cancellations present in the sum which necessitate individual Feynman diagrams to be computed to subleading orders. Moreover, it is not clear that sums of high-order Feynman diagrams with complicated criss-crossing of lines can lead to factorization implied by the multi-regge scenario. Both of these difficulties can be overcome by using the recently developed nonabelian cut diagrams. We are then able to show that the sum of ss-channel-ladder diagrams to all orders does lead to such multiple reggeon exchanges.Comment: uu-encoded latex file with 11 postscript figures (20 pages

    The Absorptive Extra Dimensions

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    It is well known that gravity and neutrino oscillation can be used to probe large extra dimensions in a braneworld scenario. We argue that neutrino oscillation remains a useful probe even when the extra dimensions are small, because the brane-bulk coupling is likely to be large. Neutrino oscillation in the presence of a strong brane-bulk coupling is vastly different from the usual case of a weak coupling. In particular, some active neutrinos could be absorbed by the bulk when they oscillate from one kind to another, a signature which can be taken as the presence of an extra dimension. In a very large class of models which we shall discuss, the amount of absorption for all neutrino oscillations is controlled by a single parameter, a property which distinguishes extra dimensions from other mechanisms for losing neutrino fluxes.Comment: Introduction enlarged; conclusions added. To appear in Phys. Rev.

    Multi-resolution processing for fractal analysis of airborne remotely sensed data

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    Fractal geometry is increasingly becoming a useful tool for modeling natural phenomenon. As an alternative to Euclidean concepts, fractals allow for a more accurate representation of the nature of complexity in natural boundaries and surfaces. Since they are characterized by self-similarity, an ideal fractal surface is scale-independent; i.e. at different scales a fractal surface looks the same. This is not exactly true for natural surfaces. When viewed at different spatial resolutions parts of natural surfaces look alike in a statistical manner and only for a limited range of scales. Images acquired by NASA's Thermal Infrared Multispectral Scanner are used to compute the fractal dimension as a function of spatial resolution. Three methods are used to determine the fractal dimension - Schelberg's line-divider method, the variogram method, and the triangular prism method. A description of these methods and the results of applying these methods to a remotely-sensed image is also presented. Five flights were flown in succession at altitudes of 2 km (low), 6 km (mid), 12 km (high), and then back again at 6 km and 2 km. The area selected was the Ross Barnett reservoir near Jackson, Mississippi. The mission was flown during the predawn hours of 1 Feb. 1992. Radiosonde data was collected for that duration to profile the characteristics of the atmosphere. This corresponds to 3 different pixel sizes - 5m, 15m, and 30m. After, simulating different spatial sampling intervals within the same image for each of the 3 image sets, the results are cross-correlated to compare the extent of detail and complexity that is obtained when data is taken at lower spatial intervals

    Integral closure of rings of integer-valued polynomials on algebras

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    Let DD be an integrally closed domain with quotient field KK. Let AA be a torsion-free DD-algebra that is finitely generated as a DD-module. For every aa in AA we consider its minimal polynomial ÎŒa(X)∈D[X]\mu_a(X)\in D[X], i.e. the monic polynomial of least degree such that ÎŒa(a)=0\mu_a(a)=0. The ring IntK(A){\rm Int}_K(A) consists of polynomials in K[X]K[X] that send elements of AA back to AA under evaluation. If DD has finite residue rings, we show that the integral closure of IntK(A){\rm Int}_K(A) is the ring of polynomials in K[X]K[X] which map the roots in an algebraic closure of KK of all the ÎŒa(X)\mu_a(X), a∈Aa\in A, into elements that are integral over DD. The result is obtained by identifying AA with a DD-subalgebra of the matrix algebra Mn(K)M_n(K) for some nn and then considering polynomials which map a matrix to a matrix integral over DD. We also obtain information about polynomially dense subsets of these rings of polynomials.Comment: Keywords: Integer-valued polynomial, matrix, triangular matrix, integral closure, pullback, polynomially dense set. accepted for publication in the volume "Commutative rings, integer-valued polynomials and polynomial functions", M. Fontana, S. Frisch and S. Glaz (editors), Springer 201

    Combinatorial Hopf algebras and Towers of Algebras

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    Bergeron and Li have introduced a set of axioms which guarantee that the Grothendieck groups of a tower of algebras ⚁n≄0An\bigoplus_{n\ge0}A_n can be endowed with the structure of graded dual Hopf algebras. Hivert and Nzeutzhap, and independently Lam and Shimozono constructed dual graded graphs from primitive elements in Hopf algebras. In this paper we apply the composition of these constructions to towers of algebras. We show that if a tower ⚁n≄0An\bigoplus_{n\ge0}A_n gives rise to graded dual Hopf algebras then we must have dim⁥(An)=rnn!\dim(A_n)=r^nn! where r=dim⁥(A1)r = \dim(A_1).Comment: 7 page

    Large Mixing Induced by the Strong Coupling with a Single Bulk Neutrinos

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    Neutrino is a good probe of extra dimensions. Large mixing and the apparent lack of very complicated oscillation patterns may be an indication of large couplings between the brane and a single bulk neutrino. A simple and realistic five-dimensional model of this kind is discussed. It requires a sterile in addition to three active neutrinos on the brane, all coupled strongly to one common bulk neutrino, but not directly among themselves. Mindful that sterile neutrinos are disfavored in the atmospheric and solar data, we demand induced mixing to occur among the active neutrinos, but not between the active and the sterile. The size RR of the extra dimension is arbitrary in this model, otherwise it contains six parameters which can be used to fit the three neutrino masses and the three mixing angles. However, in the model those six parameters must be suitably ordered, so a successful fit is not guaranteed. It turns out that not only the data can be fitted, but as a result of the ordering, a natural connection between the smallness of the reactor angle ξ13\theta_{13} and the smallness of the mass-gap ratio ΔMsolar2/ΔMatmospheric2\Delta M^2_{solar}/\Delta M^2_{atmospheric} can be derived.Comment: Misprints above eq. (22) corrected. To appear in PR
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