23,081 research outputs found

    A Proof of the Cameron-Ku conjecture

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    A family of permutations A \subset S_n is said to be intersecting if any two permutations in A agree at some point, i.e. for any \sigma, \pi \in A, there is some i such that \sigma(i)=\pi(i). Deza and Frankl showed that for such a family, |A| <= (n-1)!. Cameron and Ku showed that if equality holds then A = {\sigma \in S_{n}: \sigma(i)=j} for some i and j. They conjectured a `stability' version of this result, namely that there exists a constant c < 1 such that if A \subset S_{n} is an intersecting family of size at least c(n-1)!, then there exist i and j such that every permutation in A maps i to j (we call such a family `centred'). They also made the stronger `Hilton-Milner' type conjecture that for n \geq 6, if A \subset S_{n} is a non-centred intersecting family, then A cannot be larger than the family C = {\sigma \in S_{n}: \sigma(1)=1, \sigma(i)=i \textrm{for some} i > 2} \cup {(12)}, which has size (1-1/e+o(1))(n-1)!. We prove the stability conjecture, and also the Hilton-Milner type conjecture for n sufficiently large. Our proof makes use of the classical representation theory of S_{n}. One of our key tools will be an extremal result on cross-intersecting families of permutations, namely that for n \geq 4, if A,B \subset S_{n} are cross-intersecting, then |A||B| \leq ((n-1)!)^{2}. This was a conjecture of Leader; it was recently proved for n sufficiently large by Friedgut, Pilpel and the author.Comment: Updated version with an expanded open problems sectio

    Could a nearby supernova explosion have caused a mass extinction?

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    We examine the possibility that a nearby supernova explosion could have caused one or more of the mass extinctions identified by palaeontologists. We discuss the likely rate of such events in the light of the recent identification of Geminga as a supernova remnant less than 100 pc away and the discovery of a millisecond pulsar about 150 pc away, and observations of SN 1987A. The fluxes of γ\gamma radiation and charged cosmic rays on the Earth are estimated, and their effects on the Earth's ozone layer discussed. A supernova explosion of the order of 10 pc away could be expected every few hundred million years, and could destroy the ozone layer for hundreds of years, letting in potentially lethal solar ultraviolet radiation. In addition to effects on land ecology, this could entail mass destruction of plankton and reef communities, with disastrous consequences for marine life as well. A supernova extinction should be distinguishable from a meteorite impact such as the one that presumably killed the dinosaurs.Comment: 10 pages, CERN-TH.6805/9

    Geometric mechanics and Lagrangian reduction

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    The purpose of this thesis is two-fold: Firstly, to contribute to the tools available to geometric mechanics; secondly, to apply the geometric perspective to two particular problems. The thesis falls into three parts. The first part deals with the dynamics of charged molecular strands (CMS). The second part contributes general tools for use in geometric mechanics. The third part develops a new geometric modelling technique and applies it to image dynamics. Part I develops equations of motion for the dynamical folding of CMS (such as DNA). The CMS are modelled as flexible continuous filamentary distributions of interacting rigid charge conformations, and their dynamics are derived via a modified Hamilton-Pontryagin variational formulation. The new feature is the inclusion of nonlocal screened Coulomb interactions, or Lennard-Jones potentials between pairs of charges. The CMS equations are shown to arise from a form of Lagrangian reduction initially developed for complex fluids. Subsequently, the equations are also shown to arise from Lagrange-Poincaré reduction of a field theory. This dual interpretation of the CMS equations motivates the undertakings of Part II. In Part II, a general treatment of Lagrange-Poincaré (LP) reduction theory is undertaken. The LP equations are cast into a field theoretic context together with their associated constrained variational principle. An integrability/reconstruction condition is established that relates solutions of the original problem with those of the reduced problem. The new contribution of the LP framework is to unify the Lagrange-Poincaré field reduction with the canonical theory, which involves a single independent variable, and to extend LP field reduction to the general fibre bundle setting. The Kelvin-Noether theorem is generalised in two new ways; from the Euler- Poincaré to the LP setting, and from the canonical to the field setting. The importance of the extended Kelvin-Noether theorem is elucidated by an application to the CMS problem, yielding new qualitative insight into molecular strand dynamics. Finally, Part III gives a full geometric development of a new technique called un-reduction, that uses the canonical LP reduction back-to-front. Application of un-reduction leads to new developments in image dynamics

    Race, diversity and criminal justice in Canada:a view from the UK

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    ABSTRACT This article examines the way in which those employed in the Canadia

    Irredundant Families of Subcubes

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    We consider the problem of finding the maximum possible size of a family of k-dimensional subcubes of the n-cube {0,1}^{n}, none of which is contained in the union of the others. (We call such a family `irredundant'). Aharoni and Holzman conjectured that for k > n/2, the answer is {n choose k} (which is attained by the family of all k-subcubes containing a fixed point). We give a new proof of a general upper bound of Meshulam, and we prove that for k >= n/2, any irredundant family in which all the subcubes go through either (0,0,...,0) or (1,1,...,1) has size at most {n choose k}. We then give a general lower bound, showing that Meshulam's upper bound is always tight up to a factor of at most e.Comment: 24 page

    Intersecting Families of Permutations

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    A set of permutations ISnI \subset S_n is said to be {\em k-intersecting} if any two permutations in II agree on at least kk points. We show that for any kNk \in \mathbb{N}, if nn is sufficiently large depending on kk, then the largest kk-intersecting subsets of SnS_n are cosets of stabilizers of kk points, proving a conjecture of Deza and Frankl. We also prove a similar result concerning kk-cross-intersecting subsets. Our proofs are based on eigenvalue techniques and the representation theory of the symmetric group.Comment: 'Erratum' section added. Yuval Filmus has recently pointed out that the 'Generalised Birkhoff theorem', Theorem 29, is false for k > 1, and so is Theorem 27 for k > 1. An alternative proof of the equality part of the Deza-Frankl conjecture is referenced, bypassing the need for Theorems 27 and 2
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