Einstein Manifolds and Contact Geometry 1
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Lagrangian Intersections in Contact Geometry (First Draft)
Lagrangian intersections in contact geometry (First draft) Y. Eliashberg,∗ H. Hofer,y and D. Salamonz Stanford University∗ Ruhr-Universit¨at Bochumy Mathematics Institutez University of Warwick Coventry CV4 7AL Great Britain October 1994 1 Introduction Contact geometry Let M be a compact manifold of odd dimension 2n + 1 and ξ ⊂ T M be a contact structure. This means that ξ is an oriented field of hyperplanes and there exists a 1-form α on M such that ξ = ker α, α ^ dα^n 6= 0: The last condition means that the restriction of dα to the kernel of α is non- degenerate. Any such form is called a contact form for ξ. Any contact form determines a contact vector field (sometimes also called the Reeb vector field) Y : M ! T M via ι(Y )dα = 0; ι(Y )α = 1: A contactomorphism is a diffeomorphism : M ! M which preserves the contact structure ξ. This means that ∗α = ehα for some smooth function h : M ! . A contact isotopy is a smooth family of contactomorphisms s : M ! M such that ∗ hs s α = e α for all s. Any such isotopy with 0 = id and h0 = 0 is generated by Hamil- tonian functions Hs : M ! as follows. Each Hamiltonian function Hs determines a Hamiltonian vector field Xs = XHs = Xα,Hs : M ! T M via ι(Xs)α = −Hs; ι(Xs)dα = dHs − ι(Y )dHs · α, 1 and these vector fields determine s and hs via d d = X ◦ ; h = −ι(Y )dH : ds s s s ds s s A Legendrian submanifold of M is an n-dimensional integral submanifold L of the hyperplane field ξ, that is αjT L = 0. -
The Defocusing NLS Equation and Its Normal Form, by B. Grébert and T
BULLETIN (New Series) OF THE AMERICAN MATHEMATICAL SOCIETY Volume 53, Number 2, April 2016, Pages 337–342 http://dx.doi.org/10.1090/bull/1522 Article electronically published on October 8, 2015 The defocusing NLS equation and its normal form,byB.Gr´ebert and T. Kappeler, EMS Series of Lectures in Mathematics, European Mathematical Society (EMS), Z¨urich, 2014, x+166 pp., ISBN 978-3-03719-131-6, US$38.00 Until the end of the nineteenth century one of the major goals of differential equa- tions theory and mechanics was solving equations of motion, i.e., finding formulae that describe the time dependence of the mechanical configuration. Surprisingly enough, this has been successfully achieved in many interesting cases, such as a planet under the action of gravitation (Kepler problem, two-body problem), the motion of a free rigid body, or the motion of a symmetric rigid body under the action of gravitation (Lagrange top). All these systems are now known to belong to the general class of integrable Hamiltonian systems, for which an explicit procedure of integration of the equations was found by Liouville. Starting from the celebrated paper by Kruskal and Zabusky [ZK65], who dis- covered existence of solitons in the Kortweg–de Vries equation (KdV), mathemati- cians recognized that there are some partial differential equations that are infinite- dimensional analogs of the classical integrable systems. During the last fifty years, the techniques developed for the integration of classical finite-dimensional systems and for the study of their perturbations have been largely adapted to the case of partial differential equations (PDEs). -
Contact Geometry
Contact Geometry Hansj¨org Geiges Mathematisches Institut, Universit¨at zu K¨oln, Weyertal 86–90, 50931 K¨oln, Germany E-mail: [email protected] April 2004 Contents 1 Introduction 3 2 Contact manifolds 4 2.1 Contact manifolds and their submanifolds . 6 2.2 Gray stability and the Moser trick . 13 2.3 ContactHamiltonians . 16 2.4 Darboux’s theorem and neighbourhood theorems . 17 2.4.1 Darboux’stheorem. 17 2.4.2 Isotropic submanifolds . 19 2.4.3 Contact submanifolds . 24 2.4.4 Hypersurfaces.......................... 26 2.4.5 Applications .......................... 30 2.5 Isotopyextensiontheorems . 32 2.5.1 Isotropic submanifolds . 32 2.5.2 Contact submanifolds . 34 2.5.3 Surfaces in 3–manifolds . 36 2.6 Approximationtheorems. 37 2.6.1 Legendrianknots. 38 2.6.2 Transverseknots . 42 1 3 Contact structures on 3–manifolds 43 3.1 An invariant of transverse knots . 45 3.2 Martinet’sconstruction . 46 3.3 2–plane fields on 3–manifolds . 50 3.3.1 Hopf’s Umkehrhomomorphismus . 53 3.3.2 Representing homology classes by submanifolds . 54 3.3.3 Framedcobordisms. 56 3.3.4 Definition of the obstruction classes . 57 3.4 Let’sTwistAgain ........................... 59 3.5 Otherexistenceproofs . 64 3.5.1 Openbooks........................... 64 3.5.2 Branchedcovers ........................ 66 3.5.3 ...andmore ......................... 67 3.6 Tightandovertwisted . 67 3.7 Classificationresults . 73 4 A guide to the literature 75 4.1 Dimension3............................... 76 4.2 Higherdimensions ........................... 76 4.3 Symplecticfillings ........................... 77 4.4 DynamicsoftheReebvectorfield. 77 2 1 Introduction Over the past two decades, contact geometry has undergone a veritable meta- morphosis: once the ugly duckling known as ‘the odd-dimensional analogue of symplectic geometry’, it has now evolved into a proud field of study in its own right. -
Universal Circles for Quasigeodesic Flows 1 Introduction
Geometry & Topology 10 (2006) 2271–2298 2271 arXiv version: fonts, pagination and layout may vary from GT published version Universal circles for quasigeodesic flows DANNY CALEGARI We show that if M is a hyperbolic 3–manifold which admits a quasigeodesic flow, then π1(M) acts faithfully on a universal circle by homeomorphisms, and preserves a pair of invariant laminations of this circle. As a corollary, we show that the Thurston norm can be characterized by quasigeodesic flows, thereby generalizing a theorem of Mosher, and we give the first example of a closed hyperbolic 3–manifold without a quasigeodesic flow, answering a long-standing question of Thurston. 57R30; 37C10, 37D40, 53C23, 57M50 1 Introduction 1.1 Motivation and background Hyperbolic 3–manifolds can be studied from many different perspectives. A very fruitful perspective is to think of such manifolds as dynamical objects. For example, a very important class of hyperbolic 3–manifolds are those arising as mapping tori of pseudo-Anosov automorphisms of surfaces (Thurston [24]). Such mapping tori naturally come with a flow, the suspension flow of the automorphism. In the seminal paper [4], Cannon and Thurston showed that this suspension flow can be chosen to be quasigeodesic and pseudo-Anosov. Informally, a flow on a hyperbolic 3–manifold is quasigeodesic if the lifted flowlines in the universal cover are quasi-geodesics in H3 , and a flow is pseudo-Anosov if it looks locally like a semi-branched cover of an Anosov flow. Of course, such a flow need not be transverse to a foliation by surfaces. See Thurston [24] and Fenley [6] for background and definitions. -
Symplectic and Contact Geometry and Hamiltonian Dynamics
Symplectic and Contact Geometry and Hamiltonian Dynamics Mikhail B. Sevryuk Abstract. This is an introduction to the contributions by the lecturers at the mini-symposium on symplectic and contact geometry. We present a very general and brief account of the prehistory of the eld and give references to some seminal papers and important survey works. Symplectic geometry is the geometry of a closed nondegenerate two-form on an even-dimensional manifold. Contact geometry is the geometry of a maximally nondegenerate eld of tangent hyperplanes on an odd-dimensional manifold. The symplectic structure is fundamental for Hamiltonian dynamics, and in this sense symplectic geometry (and its odd-dimensional counterpart, contact geometry) is as old as classical mechanics. However, the science the present mini-symposium is devoted to is usually believed to date from H. Poincare’s “last geometric theo- rem” [70] concerning xed points of area-preserving mappings of an annulus: Theorem 1. (Poincare-Birkho) An area-preserving dieomorphism of an annu- lus S1[0; 1] possesses at least two xed points provided that it rotates two boundary circles in opposite directions. This theorem proven by G. D. Birkho [16] was probably the rst statement describing the properties of symplectic manifolds and symplectomorphisms “in large”, thereby giving birth to symplectic topology. In the mid 1960s [2, 3] and later in the 1970s ([4, 5, 6] and [7, Appendix 9]), V. I. Arnol’d formulated his famous conjecture generalizing Poincare’s theorem to higher dimensions. This conjecture reads as follows: Conjecture 2. (Arnol’d) A ow map A of a (possibly nonautonomous) Hamilton- ian system of ordinary dierential equations on a closed symplectic manifold M possesses at least as many xed points as a smooth function on M must have critical points, both “algebraically” and “geometrically”. -
Einstein Manifolds As Yang-Mills Instantons
arXiv:1101.5185 Einstein Manifolds As Yang-Mills Instantons a b John J. Oh ∗ and Hyun Seok Yang † a Division of Computational Sciences in Mathematics, National Institute for Mathematical Sciences, Daejeon 305-340, Korea b Institute for the Early Universe, Ewha Womans University, Seoul 120-750, Korea b Center for Quantum Spacetime, Sogang University, Seoul 121-741, Korea ABSTRACT It is well-known that Einstein gravity can be formulated as a gauge theory of Lorentz group where spin connections play a role of gauge fields and Riemann curvature tensors correspond to their field strengths. One can then pose an interesting question: What is the Einstein equation from the gauge theory point of view? Or equivalently, what is the gauge theory object corresponding to Einstein manifolds? We show that the Einstein equations in four dimensions are precisely self-duality equa- tions in Yang-Mills gauge theory and so Einstein manifolds correspond to Yang-Mills instantons in SO(4) = SU(2) SU(2) gauge theory. Specifically, we prove that any Einstein manifold L × R with or without a cosmological constant always arises as the sum of SU(2)L instantons and SU(2)R anti-instantons. This result explains why an Einstein manifold must be stable because two kinds of arXiv:1101.5185v4 [hep-th] 2 Jul 2013 instantons belong to different gauge groups, instantons in SU(2)L and anti-instantons in SU(2)R, and so they cannot decay into a vacuum. We further illuminate the stability of Einstein manifolds by showing that they carry nontrivial topological invariants. Keywords: Einstein manifold, Yang-Mills instanton, Self-duality May 30, 2018 ∗[email protected] †[email protected] 1 Introduction It seems that the essence of the method of physics is inseparably connected with the problem of interplay between local and global aspects of the world’s structure, as saliently exemplified in the index theorem of Dirac operators. -
To Be Identified. Then the Flow Line at the Origin Under the ODE System Is
4.2. LINEAR FLOWS ON THE TORUS 89 to be identified. Then the flow line at the origin under the ODE system is a straight line of slope γ emanating from the origin and meeting the right edge of the unit square at the point (1; γ). But by the identification, we can restart the graph of the line at the same height on the left side of the square (at the point (0; γ). Continuing to do this, we will eventually reach the top of the square. But by the identification again, we will drop to the bottom point and continue the line as before. See Figure 6 In essence, we are graphing the flow line as it would appear on the unit square. When we pull this square out of the plane and bend it to create our torus T, the flow line will come with it. Suppose γ ∈~ Q. What can we say about the positive flow line? Figure 6. Wrapping the flow onto T, the unit square with oppo- site sides identified. Proposition 4.16. if γ !2 is irrational, then the flow is minimal. If γ , = !1 ∈ Q then every orbit is closed. Proof. Choose a point x = (x1; x2) and let Sx be a Poincare section (a first- return map for the flow.) Then, along Sx, the Poincare map is precisely Rγ (see the left side of Figure 7). Since γ ∈~ Q, Ox ∩ Sx is dense in Sx. 2 So let y be some arbitrary point in T . We claim that arbitrarily close to y is a point in Ox. -
Eienstein Field Equations and Heisenberg's Principle Of
International Journal of Scientific and Research Publications, Volume 2, Issue 9, September 2012 1 ISSN 2250-3153 EIENSTEIN FIELD EQUATIONS AND HEISENBERG’S PRINCIPLE OF UNCERTAINLY THE CONSUMMATION OF GTR AND UNCERTAINTY PRINCIPLE 1DR K N PRASANNA KUMAR, 2PROF B S KIRANAGI AND 3PROF C S BAGEWADI ABSTRACT: The Einstein field equations (EFE) or Einstein's equations are a set of 10 equations in Albert Einstein's general theory of relativity which describe the fundamental interaction (e&eb) of gravitation as a result of space time being curved by matter and energy. First published by Einstein in 1915 as a tensor equation, the EFE equate spacetime curvature (expressed by the Einstein tensor) with (=) the energy and momentum tensor within that spacetime (expressed by the stress–energy tensor).Both space time curvature tensor and energy and momentum tensor is classified in to various groups based on which objects they are attributed to. It is to be noted that the total amount of energy and mass in the Universe is zero. But as is said in different context, it is like the Bank Credits and Debits, with the individual debits and Credits being conserved, holistically, the conservation and preservation of Debits and Credits occur, and manifest in the form of General Ledger. Transformations of energy also take place individually in the same form and if all such transformations are classified and written as a Transfer Scroll, it should tally with the total, universalistic transformation. This is a very important factor to be borne in mind. Like accounts are classifiable based on rate of interest, balance standing or the age, we can classify the factors and parameters in the Universe, be it age, interaction ability, mass, energy content. -
Hypersurfaces of Einstein Manifolds
ANNALES SCIENTIFIQUES DE L’É.N.S. NORIHITO KOISO Hypersurfaces of Einstein manifolds Annales scientifiques de l’É.N.S. 4e série, tome 14, no 4 (1981), p. 433-443 <http://www.numdam.org/item?id=ASENS_1981_4_14_4_433_0> © Gauthier-Villars (Éditions scientifiques et médicales Elsevier), 1981, tous droits réservés. L’accès aux archives de la revue « Annales scientifiques de l’É.N.S. » (http://www. elsevier.com/locate/ansens) implique l’accord avec les conditions générales d’utilisation (http://www.numdam.org/conditions). Toute utilisation commerciale ou impression systé- matique est constitutive d’une infraction pénale. Toute copie ou impression de ce fi- chier doit contenir la présente mention de copyright. Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques http://www.numdam.org/ Ann. scient. EC. Norm. Sup., 40 serie, t. 14, 1981, p. 433 a 443. HYPERSURFACES OF EINSTEIN MANIFOLDS BYNORIHITO KOISO(1) 0. Introduction and results Let (M, g) be an Einstein manifold of dimension n +1 (n ^ 2). We consider certain classes of hypersurfaces in (M, g). First, let (M, g} be a totally umbilical hypersurface in (M, g), i.e., we assume that the second fundamental form a satisfies ^=jg for some function y on M. If we know completely the curvature tensor of (M, g}, we can get much information on (M, g). For example, if(M, g) is a symmetric space, then (M, g) is also a locally symmetric space, and so the classification of such pairs [(M, g), (M, g)} reduces to Lie group theory (see Chen [4] (2), Chen and Nagano [5], Naitoh [10]). -
Hep-Th/0505211V3 12 Dec 2005 Sebasti´An Franco Brane and Tilings Geometry Toric from Theories Gauge VERSION HYPER - Style
Preprint typeset in JHEP style. - HYPER VERSION MIT-CTP-3646, CERN-PH-TH/2005-084, HUTP-05/A0027 Gauge Theories from Toric Geometry and Brane Tilings Sebasti´an Franco1, Amihay Hanany1, Dario Martelli2, James Sparks3, David Vegh1, and Brian Wecht1 1. Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. 2. Department of Physics, CERN Theory Division, 1211 Geneva 23, Switzerland. 3. Department of Mathematics, Harvard University, One Oxford Street, Cambridge, MA 02318, U.S.A. and Jefferson Physical Laboratory, Harvard University, Cambridge, MA 02138, U.S.A. [email protected], [email protected], [email protected], [email protected], [email protected], [email protected] arXiv:hep-th/0505211v3 12 Dec 2005 Abstract: We provide a general set of rules for extracting the data defining a quiver gauge theory from a given toric Calabi–Yau singularity. Our method combines information from the geometry and topology of Sasaki–Einstein manifolds, AdS/CFT, dimers, and brane tilings. We explain how the field content, quantum numbers, and superpotential of a superconformal gauge theory on D3–branes probing a toric Calabi–Yau singularity can be deduced. The infinite family of toric singularities with known horizon Sasaki–Einstein manifolds La,b,c is used to illustrate these ideas. We construct the corresponding quiver gauge theories, which may be fully specified by giving a tiling of the plane by hexagons with certain gluing rules. As checks of this construction, we perform a-maximisation as well as Z-minimisation to compute the exact R-charges of an arbitrary such quiver. We also examine a number of examples in detail, including the infinite subfamily La,b,a, whose smallest member is the Suspended Pinch Point. -
Lie Groups, Algebraic Groups and Lattices
Lie groups, algebraic groups and lattices Alexander Gorodnik Abstract This is a brief introduction to the theories of Lie groups, algebraic groups and their discrete subgroups, which is based on a lecture series given during the Summer School held in the Banach Centre in Poland in Summer 2011. Contents 1 Lie groups and Lie algebras 2 2 Invariant measures 13 3 Finite-dimensional representations 18 4 Algebraic groups 22 5 Lattices { geometric constructions 29 6 Lattices { arithmetic constructions 34 7 Borel density theorem 41 8 Suggestions for further reading 42 This exposition is an expanded version of the 10-hour course given during the first week of the Summer School \Modern dynamics and interactions with analysis, geometry and number theory" that was held in the Bedlewo Banach Centre in Summer 2011. The aim of this course was to cover background material regarding Lie groups, algebraic groups and their discrete subgroups that would be useful in the subsequent advanced courses. The presentation is 1 intended to be accessible for beginning PhD students, and we tried to make most emphasise on ideas and techniques that play fundamental role in the theory of dynamical systems. Of course, the notes would only provide one of the first steps towards mastering these topics, and in x8 we offer some suggestions for further reading. In x1 we develop the theory of (matrix) Lie groups. In particular, we introduce the notion of Lie algebra, discuss relation between Lie-group ho- momorphisms and the corresponding Lie-algebra homomorphisms, show that every Lie group has a structure of an analytic manifold, and prove that every continuous homomorphism between Lie groups is analytic. -
Contact 3-Manifolds Twenty Years Since J. Martinet's Work
ANNALES DE L’INSTITUT FOURIER YAKOV ELIASHBERG Contact 3-manifolds twenty years since J. Martinet’s work Annales de l’institut Fourier, tome 42, no 1-2 (1992), p. 165-192 <http://www.numdam.org/item?id=AIF_1992__42_1-2_165_0> © Annales de l’institut Fourier, 1992, tous droits réservés. L’accès aux archives de la revue « Annales de l’institut Fourier » (http://annalif.ujf-grenoble.fr/) implique l’accord avec les conditions gé- nérales d’utilisation (http://www.numdam.org/conditions). Toute utilisa- tion commerciale ou impression systématique est constitutive d’une in- fraction pénale. Toute copie ou impression de ce fichier doit conte- nir la présente mention de copyright. Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques http://www.numdam.org/ Ann. Inst. Fourier, Grenoble 42, 1-2 (1992), 165-192 CONTACT 3-MANIFOLDS TWENTY YEARS SINCE J. MARTINETS WORK by Yakov ELIASHBERG* To the memory of Claude GodbUlon and Jean Martinet Twenty years ago Jean Martinet (see [Ma]) showed that any orientable closed 3-manifold admits a contact structure. Three years later after the work of R. Lutz (see [4]) and in the wake of the triumph of Gromov's h- principle, it seemed that the classification of closed contact 3-manifolds was at hand. Ten years later in the seminal work [Be], D. Bennequin showed that the situation is much more complicated and that the classification of contact structures on 3-manifolds, and even on S'3, was not likely to be achieved. My paper [El] raised the hope that the situation is not so bad.