NON-EXISTENCE of METRIC on Tn with POSITIVE SCALAR
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Scalar Curvature and Geometrization Conjectures for 3-Manifolds
Comparison Geometry MSRI Publications Volume 30, 1997 Scalar Curvature and Geometrization Conjectures for 3-Manifolds MICHAEL T. ANDERSON Abstract. We first summarize very briefly the topology of 3-manifolds and the approach of Thurston towards their geometrization. After dis- cussing some general properties of curvature functionals on the space of metrics, we formulate and discuss three conjectures that imply Thurston’s Geometrization Conjecture for closed oriented 3-manifolds. The final two sections present evidence for the validity of these conjectures and outline an approach toward their proof. Introduction In the late seventies and early eighties Thurston proved a number of very re- markable results on the existence of geometric structures on 3-manifolds. These results provide strong support for the profound conjecture, formulated by Thur- ston, that every compact 3-manifold admits a canonical decomposition into do- mains, each of which has a canonical geometric structure. For simplicity, we state the conjecture only for closed, oriented 3-manifolds. Geometrization Conjecture [Thurston 1982]. Let M be a closed , oriented, 2 prime 3-manifold. Then there is a finite collection of disjoint, embedded tori Ti 2 in M, such that each component of the complement M r Ti admits a geometric structure, i.e., a complete, locally homogeneous RiemannianS metric. A more detailed description of the conjecture and the terminology will be given in Section 1. A complete Riemannian manifold N is locally homogeneous if the universal cover N˜ is a complete homogenous manifold, that is, if the isometry group Isom N˜ acts transitively on N˜. It follows that N is isometric to N=˜ Γ, where Γ is a discrete subgroup of Isom N˜, which acts freely and properly discontinuously on N˜. -
Gsm025-Endmatter.Pdf
http://dx.doi.org/10.1090/gsm/025 Selected Titles in This Series 25 Thomas Friedrich, Dirac operators in Riemannian geometry, 2000 24 Helmut Koch, Number theory: Algebraic numbers and functions, 2000 23 Alberto Candel and Lawrence Conlon, Foliations I, 2000 22 Giinter R. Krause and Thomas H. Lenagan, Growth of algebras and Gelfand-Kirillov dimension, 2000 21 John B. Conway, A course in operator theory, 2000 20 Robert E. Gompf and Andras I. Stipsicz, 4-manifolds and Kirby calculus, 1999 19 Lawrence C. Evans, Partial differential equations, 1998 18 Winfried Just and Martin Weese, Discovering modern set theory. II: Set-theoretic tools for every mathematician, 1997 17 Henryk Iwaniec, Topics in classical automorphic forms, 1997 16 Richard V. Kadison and John R. Ringrose, Fundamentals of the theory of operator algebras. Volume II: Advanced theory, 1997 15 Richard V. Kadison and John R. Ringrose, Fundamentals of the theory of operator algebras. Volume I: Elementary theory, 1997 14 Elliott H. Lieb and Michael Loss, Analysis, 1997 13 Paul C. Shields, The ergodic theory of discrete sample paths, 1996 12 N. V. Krylov, Lectures on elliptic and parabolic equations in Holder spaces, 1996 11 Jacques Dixmier, Enveloping algebras, 1996 Printing 10 Barry Simon, Representations of finite and compact groups, 1996 9 Dino Lorenzini, An invitation to arithmetic geometry, 1996 8 Winfried Just and Martin Weese, Discovering modern set theory. I: The basics, 1996 7 Gerald J. Janusz, Algebraic number fields, second edition, 1996 6 Jens Carsten Jantzen, Lectures on quantum groups, 1996 5 Rick Miranda, Algebraic curves and Riemann surfaces, 1995 4 Russell A. -
Â-Genus and Collapsing
The Journal of Geometric Analysis Volume 10, Number 3, 2000 A A-Genus and Collapsing By John Lott ABSTRACT. If M is a compact spin manifold, we give relationships between the vanishing of A( M) and the possibility that M can collapse with curvature bounded below. 1. Introduction The purpose of this paper is to extend the following simple lemma. Lemma 1.I. If M is a connectedA closed Riemannian spin manifold of nonnegative sectional curvature with dim(M) > 0, then A(M) = O. Proof Let K denote the sectional curvature of M and let R denote its scalar curvature. Suppose that A(M) (: O. Let D denote the Dirac operator on M. From the Atiyah-Singer index theorem, there is a nonzero spinor field 7t on M such that D~p = 0. From Lichnerowicz's theorem, 0 = IDOl 2 dvol = IV~Pl 2 dvol + ~- I•12 dvol. (1.1) From our assumptions, R > 0. Hence V~p = 0. This implies that I~k F2 is a nonzero constant function on M and so we must also have R = 0. Then as K > 0, we must have K = 0. This implies, from the integral formula for A'(M) [14, p. 231], that A"(M) = O. [] The spin condition is necessary in Lemma 1.l, as can be seen in the case of M = CP 2k. The Ricci-analog of Lemma 1.1 is false, as can be seen in the case of M = K3. Definition 1.2. A connected closed manifold M is almost-nonnegatively-curved if for every E > 0, there is a Riemannian metric g on M such that K(M, g) diam(M, g)2 > -E. -
Gsm038-Endmatter.Pdf
http://dx.doi.org/10.1090/gsm/038 Selected Titles in This Series 38 Elton P. Hsu, Stochastic analysis on manifolds, 2002 37 Hershel M. Farkas and Irwin Kra, Theta constants, Riemann surfaces and the modular group, 2001 36 Martin Schechter, Principles of functional analysis, second edition, 2002 35 James F. Davis and Paul Kirk, Lecture notes in algebraic topology, 2001 34 Sigurdur Helgason, Differential geometry, Lie groups, and symmetric spaces, 2001 33 Dmitri Burago, Yuri Burago, and Sergei Ivanov, A course in metric geometry, 2001 32 Robert G. Bartle, A modern theory of integration, 2001 31 Ralf Korn and Elke Korn, Option pricing and portfolio optimization: Modern methods of financial mathematics, 2001 30 J. C. McConnell and J. C. Robson, Noncommutative Noetherian rings, 2001 29 Javier Duoandikoetxea, Fourier analysis, 2001 28 Liviu I. Nicolaescu, Notes on Seiberg-Witten theory, 2000 27 Thierry Aubin, A course in differential geometry, 2001 26 Rolf Berndt, An introduction to symplectic geometry, 2001 25 Thomas Friedrich, Dirac operators in Riemannian geometry, 2000 24 Helmut Koch, Number theory: Algebraic numbers and functions, 2000 23 Alberto Candel and Lawrence Conlon, Foliations I, 2000 22 Giinter R. Krause and Thomas H. Lenagan, Growth of algebras and Gelfand-Kirillov dimension, 2000 21 John B. Conway, A course in operator theory, 2000 20 Robert E. Gompf and Andras I. Stipsicz, 4-manifolds and Kirby calculus, 1999 19 Lawrence C. Evans, Partial differential equations, 1998 18 Winfried Just and Martin Weese, Discovering modern set theory. II: Set-theoretic tools for every mathematician, 1997 17 Henryk Iwaniec, Topics in classical automorphic forms, 1997 16 Richard V. -
Differential Geometry: Curvature and Holonomy Austin Christian
University of Texas at Tyler Scholar Works at UT Tyler Math Theses Math Spring 5-5-2015 Differential Geometry: Curvature and Holonomy Austin Christian Follow this and additional works at: https://scholarworks.uttyler.edu/math_grad Part of the Mathematics Commons Recommended Citation Christian, Austin, "Differential Geometry: Curvature and Holonomy" (2015). Math Theses. Paper 5. http://hdl.handle.net/10950/266 This Thesis is brought to you for free and open access by the Math at Scholar Works at UT Tyler. It has been accepted for inclusion in Math Theses by an authorized administrator of Scholar Works at UT Tyler. For more information, please contact [email protected]. DIFFERENTIAL GEOMETRY: CURVATURE AND HOLONOMY by AUSTIN CHRISTIAN A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science Department of Mathematics David Milan, Ph.D., Committee Chair College of Arts and Sciences The University of Texas at Tyler May 2015 c Copyright by Austin Christian 2015 All rights reserved Acknowledgments There are a number of people that have contributed to this project, whether or not they were aware of their contribution. For taking me on as a student and learning differential geometry with me, I am deeply indebted to my advisor, David Milan. Without himself being a geometer, he has helped me to develop an invaluable intuition for the field, and the freedom he has afforded me to study things that I find interesting has given me ample room to grow. For introducing me to differential geometry in the first place, I owe a great deal of thanks to my undergraduate advisor, Robert Huff; our many fruitful conversations, mathematical and otherwise, con- tinue to affect my approach to mathematics. -
General Relativity Fall 2019 Lecture 11: the Riemann Tensor
General Relativity Fall 2019 Lecture 11: The Riemann tensor Yacine Ali-Ha¨ımoud October 8th 2019 The Riemann tensor quantifies the curvature of spacetime, as we will see in this lecture and the next. RIEMANN TENSOR: BASIC PROPERTIES α γ Definition { Given any vector field V , r[αrβ]V is a tensor field. Let us compute its components in some coordinate system: σ σ λ σ σ λ r[µrν]V = @[µ(rν]V ) − Γ[µν]rλV + Γλ[µrν]V σ σ λ σ λ λ ρ = @[µ(@ν]V + Γν]λV ) + Γλ[µ @ν]V + Γν]ρV 1 = @ Γσ + Γσ Γρ V λ ≡ Rσ V λ; (1) [µ ν]λ ρ[µ ν]λ 2 λµν where all partial derivatives of V µ cancel out after antisymmetrization. σ Since the left-hand side is a tensor field and V is a vector field, we conclude that R λµν is a tensor field as well { this is the tensor division theorem, which I encourage you to think about on your own. You can also check that explicitly from the transformation law of Christoffel symbols. This is the Riemann tensor, which measures the non-commutation of second derivatives of vector fields { remember that second derivatives of scalar fields do commute, by assumption. It is completely determined by the metric, and is linear in its second derivatives. Expression in LICS { In a LICS the Christoffel symbols vanish but not their derivatives. Let us compute the latter: 1 1 @ Γσ = @ gσδ (@ g + @ g − @ g ) = ησδ (@ @ g + @ @ g − @ @ g ) ; (2) µ νλ 2 µ ν λδ λ νδ δ νλ 2 µ ν λδ µ λ νδ µ δ νλ since the first derivatives of the metric components (thus of its inverse as well) vanish in a LICS. -
On the Structure of Manifolds with Positive Scalar Curvature
manuscripta manuscripta math. 28, 159 - 183 (1979) mathematica by Springef-Verlag 1979 ON THE STRUCTURE OF MANIFOLDS WITH POSITIVE SCALAR CURVATURE R. Schoen and S.T. Yau ~ Dedicated to Hans Lewy and Charles B. Morrey, Jr. In this paper, we study the question of which compact manifolds admit a metric with positive scalar curvature. Scalar curvature is perhaps the weakest invariant among all the well-known invariants constructed from the curvature tensor. It measures the deviation of the Riemannian volume of the geodesic ball from the euclidean volume of the geodesic ball. As a result, it does not tell us much of the behavior of the geodesics in the manifold. Therefore it was remarkable that in 1963, Lichnerowicz [i] was able to prove the theorem that on a compact spin manifold with positive scalar curvature, there is no harmonic spinor. Applying ^ the theorem of Atiyah-Singer, it then follows that the A-genus of the manifold is zero. Later, Hitchin [2] found that the vanish- ing theorem of Lichnerowicz can also be used to prove the other KO-characteristic numbers defined by Milnor [3] are zero. For a while, it was not clear whether these are the only topological obstructions for the existence of metrics with positive scalar curvature. It was not until 1977 that the authors found Research supported in part by NSF MCF 7804872. 0025-2611/79/0028/0159/$05.OO 159 2 SCHOEN-YAU another topological obstruction in connection with some problems in general relativity. (See [4], [5], [6].) At that time, we restricted our attention to three dimensional manifolds. -
THE DIRAC OPERATOR 1. First Properties 1.1. Definition. Let X Be A
THE DIRAC OPERATOR AKHIL MATHEW 1. First properties 1.1. Definition. Let X be a Riemannian manifold. Then the tangent bundle TX is a bundle of real inner product spaces, and we can form the corresponding Clifford bundle Cliff(TX). By definition, the bundle Cliff(TX) is a vector bundle of Z=2-graded R-algebras such that the fiber Cliff(TX)x is just the Clifford algebra Cliff(TxX) (for the inner product structure on TxX). Definition 1. A Clifford module on X is a vector bundle V over X together with an action Cliff(TX) ⊗ V ! V which makes each fiber Vx into a module over the Clifford algebra Cliff(TxX). Suppose now that V is given a connection r. Definition 2. The Dirac operator D on V is defined in local coordinates by sending a section s of V to X Ds = ei:rei s; for feig a local orthonormal frame for TX and the multiplication being Clifford multiplication. It is easy to check that this definition is independent of the coordinate system. A more invariant way of defining it is to consider the composite of differential operators (1) V !r T ∗X ⊗ V ' TX ⊗ V,! Cliff(TX) ⊗ V ! V; where the first map is the connection, the second map is the isomorphism T ∗X ' TX determined by the Riemannian structure, the third map is the natural inclusion, and the fourth map is Clifford multiplication. The Dirac operator is clearly a first-order differential operator. We can work out its symbol fairly easily. The symbol1 of the connection r is ∗ Sym(r)(v; t) = iv ⊗ t; v 2 Vx; t 2 Tx X: All the other differential operators in (1) are just morphisms of vector bundles. -
Introduction
Introduction Spin Geometry is the hidden facet of Riemannian Geometry. It arises from the representation theory of the special orthogonal group SOn, more precisely, from the spinor representation, a certain representation of the Lie algebra son which is not a representation of SOn. Spinors can always be constructed locally on a given Riemannian manifold, but globally there are topological obstructions for their exis- tence. Spin Geometry lies therefore at the cross-road of several subelds of modern Mathematics. Algebra, Geometry, Topology, and Analysis are subtly interwoven in the theory of spinors, both in their denition and in their applications. Spinors have also greatly inuenced Theoretical Physics, which is nowadays one of the main driv- ing forces fostering their formidable development. The Noncommutative Geometry of Alain Connes has at its core the Dirac operator on spinors. The same Dirac operator is at the heart of the Atiyah–Singer index formula for elliptic operators on compact manifolds, linking in a spectacular way the topology of a manifold to the space of solutions to elliptic equations. Signicantly, the classical Riemann–Roch formula and its generalization by Hirzebruch; the Gauß–Bonnet formula and its extension by Chern; and nally Hirzebruch’s topological signature theorem, provide most of the examples in the index formula, but it was the Dirac operator acting on spinors which turned out to be the keystone of the index formula, both in its formulation and in its subsequent developments. The Dirac operator appears to be the primordial example of an elliptic operator, while spinors, although younger than differential forms or tensors, illustrate once again that aux âmes bien nées, la valeur n’attend point le nombre des années. -
Riemannian Submanifolds: a Survey
RIEMANNIAN SUBMANIFOLDS: A SURVEY BANG-YEN CHEN Contents Chapter 1. Introduction .............................. ...................6 Chapter 2. Nash’s embedding theorem and some related results .........9 2.1. Cartan-Janet’s theorem .......................... ...............10 2.2. Nash’s embedding theorem ......................... .............11 2.3. Isometric immersions with the smallest possible codimension . 8 2.4. Isometric immersions with prescribed Gaussian or Gauss-Kronecker curvature .......................................... ..................12 2.5. Isometric immersions with prescribed mean curvature. ...........13 Chapter 3. Fundamental theorems, basic notions and results ...........14 3.1. Fundamental equations ........................... ..............14 3.2. Fundamental theorems ............................ ..............15 3.3. Basic notions ................................... ................16 3.4. A general inequality ............................. ...............17 3.5. Product immersions .............................. .............. 19 3.6. A relationship between k-Ricci tensor and shape operator . 20 3.7. Completeness of curvature surfaces . ..............22 Chapter 4. Rigidity and reduction theorems . ..............24 4.1. Rigidity ....................................... .................24 4.2. A reduction theorem .............................. ..............25 Chapter 5. Minimal submanifolds ....................... ...............26 arXiv:1307.1875v1 [math.DG] 7 Jul 2013 5.1. First and second variational formulas -
Riemannian Holonomy and Algebraic Geometry
Riemannian Holonomy and Algebraic Geometry Arnaud BEAUVILLE Revised version (March 2006) Introduction This survey is devoted to a particular instance of the interaction between Riemannian geometry and algebraic geometry, the study of manifolds with special holonomy. The holonomy group is one of the most basic objects associated with a Riemannian metric; roughly, it tells us what are the geometric objects on the manifold (complex structures, differential forms, ...) which are parallel with respect to the metric (see 1.3 for a precise statement). There are two surprising facts about this group. The first one is that, despite its very general definition, there are few possibilities – this is Berger’s theorem (1.2). The second one is that apart from the generic case in which the holonomy group is SO(n) , all other cases appear to be related in some way to algebraic geometry. Indeed the study of compact manifolds with special holonomy brings into play some special, and quite interesting, classes of algebraic varieties: Calabi-Yau, complex symplectic or complex contact manifolds. I would like to convince algebraic geometers that this interplay is interesting on two accounts: on one hand the general theorems on holonomy give deep results on the geometry of these special varieties; on the other hand Riemannian geometry provides us with good problems in algebraic geometry – see 4.3 for a typical example. I have tried to make these notes accessible to students with little knowledge of Riemannian geometry, and a basic knowledge of algebraic geometry. Two appendices at the end recall the basic results of Riemannian (resp. -
The Einstein Tensor Characterizing Some Riemann Spaces
••fc IC/93/204 Internal Report (Limited Distribution) International Atomic Energy Agency and United Nations Educational Scientific and Cultural Organization INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS THE EINSTEIN TENSOR CHARACTERIZING SOME RIEMANN SPACES M. S. Rahman1 International Centre for Theoretical Physics, Trieste, Italy. ABSTRACT A formal definition of the Einstein tensor is given. Mention is made of how this tensor plays a role of expressing certain conditions in a precise form. The cases of reducing the Einstein tensor to a zero tensor are studied on its merit. A lucid account of results, formulated as theorems, on Einstein symmetric and Einstein recurrent spaces is then presented. MIRAMARE - TRIESTE July 1993 Permanent address: Department of Mathematics, Jahangirnagar University, Savar, Dhaka-134;2, Bangladesh. 1 Introduction and Definition The Einstein tensor [5] is defined by This tensor is in covariant form E R (1) We note that Exjj — 0 which means that the divergence of the Einstein tensor vanishes. This equation which is very remarkably an identity in Riemannian geometry is impor- tant in the theory of Relativity. Einstein's tensor has proved of tremendous importance for subsequent researches both in Riemannian geometry and in Relativity. Hitherto, the tensor had been of interest to mathematicians and physicists, and simply for its own sake. Contracting (1) with gl> gives E = R-^R where we may call E the Einstein scalar curvature. It readily follows from (2) that in a V4 the algebraic sum of the Einstein scalar curva- ture and scalar curvature is zero, that is, E + R = 0. This paper illuminates the virtue of the Einstein tensor in a consistent manner and deals with its characterizing some Riemann spaces.