331 research outputs found

    A note on entropy estimation

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    We compare an entropy estimator HzH_z recently discussed in [10] with two estimators H1H_1 and H2H_2 introduced in [6][7]. We prove the identity Hz≡H1H_z \equiv H_1, which has not been taken into account in [10]. Then, we prove that the statistical bias of H1H_1 is less than the bias of the ordinary likelihood estimator of entropy. Finally, by numerical simulation we verify that for the most interesting regime of small sample estimation and large event spaces, the estimator H2H_2 has a significant smaller statistical error than HzH_z.Comment: 7 pages, including 4 figures; two references adde

    On the uncertainty principle in Rindler and Friedmann spacetimes

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    We revise the extended uncertainty relations for the Rindler and Friedmann spacetimes recently discussed by Dabrowski and Wagner in [9]. We reveal these results to be coordinate dependent expressions of the invariant uncertainty relations recently derived for general 3-dimensional spaces of constant curvature in [10]. Moreover, we show that the non-zero minimum standard deviations of the momentum in [9] are just artifacts caused by an unfavorable choice of coordinate systems which can be removed by standard arguments of geodesic completion

    A reinterpretation of the cosmological vacuum

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    In this paper, we make a proposal for addressing the cosmological constant problem. Our approach will be based on a reinterpretation of two non-standard de Sitter solutions given by the Einstein vacuum equations with Λ\u3e0. As a first result, we derive an uncertainty principle for both variants of the de Sitter space (Theorem). Subsequently, a decomposition of the cosmological constant in a pair of time-dependent pieces is introduced (Corollary). The time-dependence of the corresponding energy and dark energy density is discussed and especially matched at the Planck scale. Furthermore, we show that for every instant of cosmic time this approach can be revealed in terms of a Schwarzschild-Anti-de Sitter cosmology with Λ\u3e0. The corresponding field equations are provided

    The predictability of letters in written english

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    We show that the predictability of letters in written English texts depends strongly on their position in the word. The first letters are usually the least easy to predict. This agrees with the intuitive notion that words are well defined subunits in written languages, with much weaker correlations across these units than within them. It implies that the average entropy of a letter deep inside a word is roughly 4 times smaller than the entropy of the first letter.Comment: 3 pages, 4 figure

    On Lattice-Free Orbit Polytopes

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    Given a permutation group acting on coordinates of Rn\mathbb{R}^n, we consider lattice-free polytopes that are the convex hull of an orbit of one integral vector. The vertices of such polytopes are called \emph{core points} and they play a key role in a recent approach to exploit symmetry in integer convex optimization problems. Here, naturally the question arises, for which groups the number of core points is finite up to translations by vectors fixed by the group. In this paper we consider transitive permutation groups and prove this type of finiteness for the 22-homogeneous ones. We provide tools for practical computations of core points and obtain a complete list of representatives for all 22-homogeneous groups up to degree twelve. For transitive groups that are not 22-homogeneous we conjecture that there exist infinitely many core points up to translations by the all-ones-vector. We prove our conjecture for two large classes of groups: For imprimitive groups and groups that have an irrational invariant subspace.Comment: 27 pages, 2 figures; with minor adaptions according to referee comments; to appear in Discrete and Computational Geometr
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