Lecture 3 Outline
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Metric Geometry in a Tame Setting
University of California Los Angeles Metric Geometry in a Tame Setting A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Mathematics by Erik Walsberg 2015 c Copyright by Erik Walsberg 2015 Abstract of the Dissertation Metric Geometry in a Tame Setting by Erik Walsberg Doctor of Philosophy in Mathematics University of California, Los Angeles, 2015 Professor Matthias J. Aschenbrenner, Chair We prove basic results about the topology and metric geometry of metric spaces which are definable in o-minimal expansions of ordered fields. ii The dissertation of Erik Walsberg is approved. Yiannis N. Moschovakis Chandrashekhar Khare David Kaplan Matthias J. Aschenbrenner, Committee Chair University of California, Los Angeles 2015 iii To Sam. iv Table of Contents 1 Introduction :::::::::::::::::::::::::::::::::::::: 1 2 Conventions :::::::::::::::::::::::::::::::::::::: 5 3 Metric Geometry ::::::::::::::::::::::::::::::::::: 7 3.1 Metric Spaces . 7 3.2 Maps Between Metric Spaces . 8 3.3 Covers and Packing Inequalities . 9 3.3.1 The 5r-covering Lemma . 9 3.3.2 Doubling Metrics . 10 3.4 Hausdorff Measures and Dimension . 11 3.4.1 Hausdorff Measures . 11 3.4.2 Hausdorff Dimension . 13 3.5 Topological Dimension . 15 3.6 Left-Invariant Metrics on Groups . 15 3.7 Reductions, Ultralimits and Limits of Metric Spaces . 16 3.7.1 Reductions of Λ-valued Metric Spaces . 16 3.7.2 Ultralimits . 17 3.7.3 GH-Convergence and GH-Ultralimits . 18 3.7.4 Asymptotic Cones . 19 3.7.5 Tangent Cones . 22 3.7.6 Conical Metric Spaces . 22 3.8 Normed Spaces . 23 4 T-Convexity :::::::::::::::::::::::::::::::::::::: 24 4.1 T-convex Structures . -
Analysis in Metric Spaces Mario Bonk, Luca Capogna, Piotr Hajłasz, Nageswari Shanmugalingam, and Jeremy Tyson
Analysis in Metric Spaces Mario Bonk, Luca Capogna, Piotr Hajłasz, Nageswari Shanmugalingam, and Jeremy Tyson study of quasiconformal maps on such boundaries moti- The authors of this piece are organizers of the AMS vated Heinonen and Koskela [HK98] to axiomatize several 2020 Mathematics Research Communities summer aspects of Euclidean quasiconformal geometry in the set- conference Analysis in Metric Spaces, one of five ting of metric measure spaces and thereby extend Mostow’s topical research conferences offered this year that are work beyond the sub-Riemannian setting. The ground- focused on collaborative research and professional breaking work [HK98] initiated the modern theory of anal- development for early-career mathematicians. ysis on metric spaces. Additional information can be found at https://www Analysis on metric spaces is nowadays an active and in- .ams.org/programs/research-communities dependent field, bringing together researchers from differ- /2020MRC-MetSpace. Applications are open until ent parts of the mathematical spectrum. It has far-reaching February 15, 2020. applications to areas as diverse as geometric group the- ory, nonlinear PDEs, and even theoretical computer sci- The subject of analysis, more specifically, first-order calcu- ence. As a further sign of recognition, analysis on met- lus, in metric measure spaces provides a unifying frame- ric spaces has been included in the 2010 MSC classifica- work for ideas and questions from many different fields tion as a category (30L: Analysis on metric spaces). In this of mathematics. One of the earliest motivations and ap- short survey, we can discuss only a small fraction of areas plications of this theory arose in Mostow’s work [Mos73], into which analysis on metric spaces has expanded. -
Metric Spaces We Have Talked About the Notion of Convergence in R
Mathematics Department Stanford University Math 61CM – Metric spaces We have talked about the notion of convergence in R: Definition 1 A sequence an 1 of reals converges to ` R if for all " > 0 there exists N N { }n=1 2 2 such that n N, n N implies an ` < ". One writes lim an = `. 2 ≥ | − | With . the standard norm in Rn, one makes the analogous definition: k k n n Definition 2 A sequence xn 1 of points in R converges to x R if for all " > 0 there exists { }n=1 2 N N such that n N, n N implies xn x < ". One writes lim xn = x. 2 2 ≥ k − k One important consequence of the definition in either case is that limits are unique: Lemma 1 Suppose lim xn = x and lim xn = y. Then x = y. Proof: Suppose x = y.Then x y > 0; let " = 1 x y .ThusthereexistsN such that n N 6 k − k 2 k − k 1 ≥ 1 implies x x < ", and N such that n N implies x y < ". Let n = max(N ,N ). Then k n − k 2 ≥ 2 k n − k 1 2 x y x x + x y < 2" = x y , k − kk − nk k n − k k − k which is a contradiction. Thus, x = y. ⇤ Note that the properties of . were not fully used. What we needed is that the function d(x, y)= k k x y was non-negative, equal to 0 only if x = y,symmetric(d(x, y)=d(y, x)) and satisfied the k − k triangle inequality. -
Euclidean Space - Wikipedia, the Free Encyclopedia Page 1 of 5
Euclidean space - Wikipedia, the free encyclopedia Page 1 of 5 Euclidean space From Wikipedia, the free encyclopedia In mathematics, Euclidean space is the Euclidean plane and three-dimensional space of Euclidean geometry, as well as the generalizations of these notions to higher dimensions. The term “Euclidean” distinguishes these spaces from the curved spaces of non-Euclidean geometry and Einstein's general theory of relativity, and is named for the Greek mathematician Euclid of Alexandria. Classical Greek geometry defined the Euclidean plane and Euclidean three-dimensional space using certain postulates, while the other properties of these spaces were deduced as theorems. In modern mathematics, it is more common to define Euclidean space using Cartesian coordinates and the ideas of analytic geometry. This approach brings the tools of algebra and calculus to bear on questions of geometry, and Every point in three-dimensional has the advantage that it generalizes easily to Euclidean Euclidean space is determined by three spaces of more than three dimensions. coordinates. From the modern viewpoint, there is essentially only one Euclidean space of each dimension. In dimension one this is the real line; in dimension two it is the Cartesian plane; and in higher dimensions it is the real coordinate space with three or more real number coordinates. Thus a point in Euclidean space is a tuple of real numbers, and distances are defined using the Euclidean distance formula. Mathematicians often denote the n-dimensional Euclidean space by , or sometimes if they wish to emphasize its Euclidean nature. Euclidean spaces have finite dimension. Contents 1 Intuitive overview 2 Real coordinate space 3 Euclidean structure 4 Topology of Euclidean space 5 Generalizations 6 See also 7 References Intuitive overview One way to think of the Euclidean plane is as a set of points satisfying certain relationships, expressible in terms of distance and angle. -
Distance Metric Learning, with Application to Clustering with Side-Information
Distance metric learning, with application to clustering with side-information Eric P. Xing, Andrew Y. Ng, Michael I. Jordan and Stuart Russell University of California, Berkeley Berkeley, CA 94720 epxing,ang,jordan,russell ¡ @cs.berkeley.edu Abstract Many algorithms rely critically on being given a good metric over their inputs. For instance, data can often be clustered in many “plausible” ways, and if a clustering algorithm such as K-means initially fails to find one that is meaningful to a user, the only recourse may be for the user to manually tweak the metric until sufficiently good clusters are found. For these and other applications requiring good metrics, it is desirable that we provide a more systematic way for users to indicate what they con- sider “similar.” For instance, we may ask them to provide examples. In this paper, we present an algorithm that, given examples of similar (and, if desired, dissimilar) pairs of points in ¢¤£ , learns a distance metric over ¢¥£ that respects these relationships. Our method is based on posing met- ric learning as a convex optimization problem, which allows us to give efficient, local-optima-free algorithms. We also demonstrate empirically that the learned metrics can be used to significantly improve clustering performance. 1 Introduction The performance of many learning and datamining algorithms depend critically on their being given a good metric over the input space. For instance, K-means, nearest-neighbors classifiers and kernel algorithms such as SVMs all need to be given good metrics that -
Distance Between Points on the Earth's Surface
Distance between Points on the Earth's Surface Abstract During a casual conversation with one of my students, he asked me how one could go about computing the distance between two points on the surface of the Earth, in terms of their respective latitudes and longitudes. This is an interesting exercise in spherical coordinates, and relates to the so-called haversine. The calculation of the distance be- tween two points on the surface of the Spherical coordinates Earth proceeds in two stages: (1) to z compute the \straight-line" Euclidean x=Rcosθcos φ distance these two points (obtained by y=Rcosθsin φ R burrowing through the Earth), and (2) z=Rsinθ to convert this distance to one mea- θ y sured along the surface of the Earth. φ Figure 1 depicts the spherical coor- dinates we shall use.1 We orient this coordinate system so that x Figure 1: Spherical Coordinates (i) The origin is at the Earth's center; (ii) The x-axis passes through the Prime Meridian (0◦ longitude); (iii) The xy-plane contains the Earth's equator (and so the positive z-axis will pass through the North Pole) Note that the angle θ is the measurement of lattitude, and the angle φ is the measurement of longitude, where 0 ≤ φ < 360◦, and −90◦ ≤ θ ≤ 90◦. Negative values of θ correspond to points in the Southern Hemisphere, and positive values of θ correspond to points in the Northern Hemisphere. When one uses spherical coordinates it is typical for the radial distance R to vary; however, in our discussion we may fix it to be the average radius of the Earth: R ≈ 6; 378 km: 1What is depicted are not the usual spherical coordinates, as the angle θ is usually measure from the \zenith", or z-axis. -
5.2. Inner Product Spaces 1 5.2
5.2. Inner Product Spaces 1 5.2. Inner Product Spaces Note. In this section, we introduce an inner product on a vector space. This will allow us to bring much of the geometry of Rn into the infinite dimensional setting. Definition 5.2.1. A vector space with complex scalars hV, Ci is an inner product space (also called a Euclidean Space or a Pre-Hilbert Space) if there is a function h·, ·i : V × V → C such that for all u, v, w ∈ V and a ∈ C we have: (a) hv, vi ∈ R and hv, vi ≥ 0 with hv, vi = 0 if and only if v = 0, (b) hu, v + wi = hu, vi + hu, wi, (c) hu, avi = ahu, vi, and (d) hu, vi = hv, ui where the overline represents the operation of complex conju- gation. The function h·, ·i is called an inner product. Note. Notice that properties (b), (c), and (d) of Definition 5.2.1 combine to imply that hu, av + bwi = ahu, vi + bhu, wi and hau + bv, wi = ahu, wi + bhu, wi for all relevant vectors and scalars. That is, h·, ·i is linear in the second positions and “conjugate-linear” in the first position. 5.2. Inner Product Spaces 2 Note. We can also define an inner product on a vector space with real scalars by requiring that h·, ·i : V × V → R and by replacing property (d) in Definition 5.2.1 with the requirement that the inner product is symmetric: hu, vi = hv, ui. Then Rn with the usual dot product is an example of a real inner product space. -
Learning a Distance Metric from Relative Comparisons
Learning a Distance Metric from Relative Comparisons Matthew Schultz and Thorsten Joachims Department of Computer Science Cornell University Ithaca, NY 14853 schultz,tj @cs.cornell.edu Abstract This paper presents a method for learning a distance metric from rel- ative comparison such as “A is closer to B than A is to C”. Taking a Support Vector Machine (SVM) approach, we develop an algorithm that provides a flexible way of describing qualitative training data as a set of constraints. We show that such constraints lead to a convex quadratic programming problem that can be solved by adapting standard meth- ods for SVM training. We empirically evaluate the performance and the modelling flexibility of the algorithm on a collection of text documents. 1 Introduction Distance metrics are an essential component in many applications ranging from supervised learning and clustering to product recommendations and document browsing. Since de- signing such metrics by hand is difficult, we explore the problem of learning a metric from examples. In particular, we consider relative and qualitative examples of the form “A is closer to B than A is to C”. We believe that feedback of this type is more easily available in many application setting than quantitative examples (e.g. “the distance between A and B is 7.35”) as considered in metric Multidimensional Scaling (MDS) (see [4]), or absolute qualitative feedback (e.g. “A and B are similar”, “A and C are not similar”) as considered in [11]. Building on the study in [7], search-engine query logs are one example where feedback of the form “A is closer to B than A is to C” is readily available for learning a (more semantic) similarity metric on documents. -
LAB 9.1 Taxicab Versus Euclidean Distance
([email protected] LAB 9.1 Name(s) Taxicab Versus Euclidean Distance Equipment: Geoboard, graph or dot paper If you can travel only horizontally or vertically (like a taxicab in a city where all streets run North-South and East-West), the distance you have to travel to get from the origin to the point (2, 3) is 5.This is called the taxicab distance between (0, 0) and (2, 3). If, on the other hand, you can go from the origin to (2, 3) in a straight line, the distance you travel is called the Euclidean distance, or just the distance. Finding taxicab distance: Taxicab distance can be measured between any two points, whether on a street or not. For example, the taxicab distance from (1.2, 3.4) to (9.9, 9.9) is the sum of 8.7 (the horizontal component) and 6.5 (the vertical component), for a total of 15.2. 1. What is the taxicab distance from (2, 3) to the following points? a. (7, 9) b. (–3, 8) c. (2, –1) d. (6, 5.4) e. (–1.24, 3) f. (–1.24, 5.4) Finding Euclidean distance: There are various ways to calculate Euclidean distance. Here is one method that is based on the sides and areas of squares. Since the area of the square at right is y 13 (why?), the side of the square—and therefore the Euclidean distance from, say, the origin to the point (2,3)—must be ͙ෆ13,or approximately 3.606 units. 3 x 2 Geometry Labs Section 9 Distance and Square Root 121 © 1999 Henri Picciotto, www.MathEducationPage.org ([email protected] LAB 9.1 Name(s) Taxicab Versus Euclidean Distance (continued) 2. -
Section 20. the Metric Topology
20. The Metric Topology 1 Section 20. The Metric Topology Note. The topological concepts you encounter in Analysis 1 are based on the metric on R which gives the distance between x and y in R which gives the distance between x and y in R as |x − y|. More generally, any space with a metric on it can have a topology defined in terms of the metric (which is ultimately based on an ε definition of pen sets). This is done in our Complex Analysis 1 (MATH 5510) class (see the class notes for Chapter 2 of http://faculty.etsu.edu/gardnerr/5510/notes. htm). In this section we define a metric and use it to create the “metric topology” on a set. Definition. A metric on a set X is a function d : X × X → R having the following properties: (1) d(x, y) ≥ 0 for all x, y ∈ X and d(x, y) = 0 if and only if x = y. (2) d(x, y)= d(y, x) for all x, y ∈ X. (3) (The Triangle Inequality) d(x, y)+ d(y, z) ≥ d(x, z) for all x, y, z ∈ X. The nonnegative real number d(x, y) is the distance between x and y. Set X together with metric d form a metric space. Define the set Bd(x, ε)= {y | d(x, y) < ε}, called the ε-ball centered at x (often simply denoted B(x, ε)). Definition. If d is a metric on X then the collection of all ε-balls Bd(x, ε) for x ∈ X and ε> 0 is a basis for a topology on X, called the metric topology induced by d. -
Contraction Principles in $ M S $-Metric Spaces
Contraction Principles in Ms-metric Spaces N. Mlaiki1, N. Souayah2, K. Abodayeh3, T. Abdeljawad4 Department of Mathematical Sciences, Prince Sultan University1,3,4 Department of Natural Sciences, Community College, King Saud University2 Riyadh, Saudi Arabia 11586 E-mail: [email protected] [email protected] [email protected] [email protected] Abstract In this paper, we give an interesting extension of the partial S-metric space which was introduced [4] to the Ms-metric space. Also, we prove the existence and uniqueness of a fixed point for a self mapping on an Ms-metric space under different contraction principles. 1 Introduction Many researchers over the years proved many interesting results on the existence of a fixed point for a self mapping on different types of metric spaces for example, see ([2], [3], [5], [6], [7], [8], [9], [10], [12], [17], [18], [19].) The idea behind this paper was inspired by the work of Asadi in [1]. He gave a more general extension of almost any metric space with two dimensions, and that is not just by defining the self ”distance” in a metric as in partial metric spaces [13, 14, 15, 16, 11], but he assumed that is not necessary that the self ”distance” is arXiv:1610.02582v1 [math.GM] 8 Oct 2016 less than the value of the metric between two different elements. In [4], an extension of S-metric spaces to a partial S-metric spaces was introduced. Also, they showed that every S-metric space is a partial S-metric space, but not every partial S- metric space is an S-metric space. -
SCALAR PRODUCTS, NORMS and METRIC SPACES 1. Definitions Below, “Real Vector Space” Means a Vector Space V Whose Field Of
SCALAR PRODUCTS, NORMS AND METRIC SPACES 1. Definitions Below, \real vector space" means a vector space V whose field of scalars is R, the real numbers. The main example for MATH 411 is V = Rn. Also, keep in mind that \0" is a many splendored symbol, with meaning depending on context. It could for example mean the number zero, or the zero vector in a vector space. Definition 1.1. A scalar product is a function which associates to each pair of vectors x; y from a real vector space V a real number, < x; y >, such that the following hold for all x; y; z in V and α in R: (1) < x; x > ≥ 0, and < x; x > = 0 if and only if x = 0. (2) < x; y > = < y; x >. (3) < x + y; z > = < x; z > + < y; z >. (4) < αx; y > = α < x; y >. n The dot product is defined for vectors in R as x · y = x1y1 + ··· + xnyn. The dot product is an example of a scalar product (and this is the only scalar product we will need in MATH 411). Definition 1.2. A norm on a real vector space V is a function which associates to every vector x in V a real number, jjxjj, such that the following hold for every x in V and every α in R: (1) jjxjj ≥ 0, and jjxjj = 0 if and only if x = 0. (2) jjαxjj = jαjjjxjj. (3) (Triangle Inequality for norm) jjx + yjj ≤ jjxjj + jjyjj. p The standard Euclidean norm on Rn is defined by jjxjj = x · x.