Geometric Theory of Heat from Souriau Lie Groups Thermodynamics and Koszul Hessian Geometry: Applications in Information Geometry for Exponential Families
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Coadjoint Orbits of Lie Algebras and Cartan Class
Symmetry, Integrability and Geometry: Methods and Applications SIGMA 15 (2019), 002, 20 pages Coadjoint Orbits of Lie Algebras and Cartan Class Michel GOZE y and Elisabeth REMM z y Ramm Algebra Center, 4 rue de Cluny, F-68800 Rammersmatt, France E-mail: [email protected] z Universit´ede Haute-Alsace, IRIMAS EA 7499, D´epartement de Math´ematiques, F-68100 Mulhouse, France E-mail: [email protected] Received September 13, 2018, in final form December 31, 2018; Published online January 09, 2019 https://doi.org/10.3842/SIGMA.2019.002 Abstract. We study the coadjoint orbits of a Lie algebra in terms of Cartan class. In fact, the tangent space to a coadjoint orbit O(α) at the point α corresponds to the characteristic space associated to the left invariant form α and its dimension is the even part of the Cartan class of α. We apply this remark to determine Lie algebras such that all the nontrivial orbits (nonreduced to a point) have the same dimension, in particular when this dimension is 2 or 4. We determine also the Lie algebras of dimension 2n or 2n + 1 having an orbit of dimension 2n. Key words: Lie algebras; coadjoint representation; contact forms; Frobenius Lie algebras; Cartan class 2010 Mathematics Subject Classification: 17B20; 17B30; 53D10; 53D05 1 Introduction Let G be a connected Lie group, g its Lie algebra and g∗ the dual vector space of g. We identify g with the Lie algebra of left invariant vector fields on G and g∗ with the vector space of left invariant Pfaffian forms on G. -
Moon-Earth-Sun: the Oldest Three-Body Problem
Moon-Earth-Sun: The oldest three-body problem Martin C. Gutzwiller IBM Research Center, Yorktown Heights, New York 10598 The daily motion of the Moon through the sky has many unusual features that a careful observer can discover without the help of instruments. The three different frequencies for the three degrees of freedom have been known very accurately for 3000 years, and the geometric explanation of the Greek astronomers was basically correct. Whereas Kepler’s laws are sufficient for describing the motion of the planets around the Sun, even the most obvious facts about the lunar motion cannot be understood without the gravitational attraction of both the Earth and the Sun. Newton discussed this problem at great length, and with mixed success; it was the only testing ground for his Universal Gravitation. This background for today’s many-body theory is discussed in some detail because all the guiding principles for our understanding can be traced to the earliest developments of astronomy. They are the oldest results of scientific inquiry, and they were the first ones to be confirmed by the great physicist-mathematicians of the 18th century. By a variety of methods, Laplace was able to claim complete agreement of celestial mechanics with the astronomical observations. Lagrange initiated a new trend wherein the mathematical problems of mechanics could all be solved by the same uniform process; canonical transformations eventually won the field. They were used for the first time on a large scale by Delaunay to find the ultimate solution of the lunar problem by perturbing the solution of the two-body Earth-Moon problem. -
Alexis Claude Clairaut
Alexis Claude Clairaut Born: 7 May 1713 in Paris, France Died: 17 May 1765 in Paris, France Alexis Clairaut's father, Jean-Baptiste Clairaut, taught mathematics in Paris and showed his quality by being elected to the Berlin Academy. Alexis's mother, Catherine Petit, had twenty children although only Alexis survived to adulthood. Jean-Baptiste Clairaut educated his son at home and set unbelievably high standards. Alexis used Euclid's Elements while learning to read and by the age of nine he had mastered the excellent mathematics textbook of Guisnée Application de l'algèbre à la géométrie which provided a good introduction to the differential and integral calculus as well as analytical geometry. In the following year, Clairaut went on to study de L'Hôpital's books, in particular his famous text Analyse des infiniment petits pour l'intelligence des lignes courbes. Few people have read their first paper to an academy at the age of 13, but this was the incredible achievement of Clairaut's in 1726 when he read his paper Quatre problèmes sur de nouvelles courbes to the Paris Academy. Although we have already noted that Clairaut was the only one of twenty children of his parents to reach adulthood, he did have a younger brother who, at the age of 14, read a mathematics paper to the Academy in 1730. This younger brother died in 1732 at the age of 16. Clairaut began to undertake research on double curvature curves which he completed in 1729. As a result of this work he was proposed for membership of the Paris Academy on 4 September 1729 but the king did not confirm his election until 1731. -
C*-Algebras and Kirillov's Coadjoint Orbit Method
C∗-ALGEBRAS AND KIRILLOV'S COADJOINT ORBIT METHOD DAVID SCHWEIN One of the main goals of representation theory is to understand the unitary dual of a topological group, that is, the set of irreducible unitary representations. Much of modern number theory, for instance, is concerned with describing the unitary duals of various reduc- tive groups over a local field or the adeles, and here our understanding of the representation theory is far from complete. For a different class of groups, the nilpotent Lie groups, A. A. Kirillov gave in the mid- nineteenth century [Kir62] a simple and transparent description of the unitary dual: it is the orbit space under the coadjoint action of the Lie group on the dual of its Lie algebra. The goal of this article, notes for a talk, is to explain Kirillov's result and illustrate it with the Heisenberg group, following Kirillov's excellent and approachable book on the subject [Kir04]. We begin with an introductory section on the unitary dual of a C∗-algebra, the proper setting (currently) for unitary representations of locally compact groups, following Dixmier's exhaustive monograph on C∗-algebras [Dix77]. 1. C∗-algebras and the unitary dual The theory of unitary representations of locally compact topological groups, for instance, reductive p-adic groups, is a special case of the more general theory of representations of C∗-algebras. In this section we review the representation theory of C∗-algebras and see how it specializes to that of topological groups. 1.1. Definitions and examples. A Banach algebra is a Banach space A equipped with an algebra structure with respect to which the norm is sub-multiplicative: ka · bk ≤ kak · kbk; a; b 2 A: We do note require Banach algebras to be unital, and in fact, we will see shortly that there are many natural examples that are not unital. -
Representation Theory
M392C NOTES: REPRESENTATION THEORY ARUN DEBRAY MAY 14, 2017 These notes were taken in UT Austin's M392C (Representation Theory) class in Spring 2017, taught by Sam Gunningham. I live-TEXed them using vim, so there may be typos; please send questions, comments, complaints, and corrections to [email protected]. Thanks to Kartik Chitturi, Adrian Clough, Tom Gannon, Nathan Guermond, Sam Gunningham, Jay Hathaway, and Surya Raghavendran for correcting a few errors. Contents 1. Lie groups and smooth actions: 1/18/172 2. Representation theory of compact groups: 1/20/174 3. Operations on representations: 1/23/176 4. Complete reducibility: 1/25/178 5. Some examples: 1/27/17 10 6. Matrix coefficients and characters: 1/30/17 12 7. The Peter-Weyl theorem: 2/1/17 13 8. Character tables: 2/3/17 15 9. The character theory of SU(2): 2/6/17 17 10. Representation theory of Lie groups: 2/8/17 19 11. Lie algebras: 2/10/17 20 12. The adjoint representations: 2/13/17 22 13. Representations of Lie algebras: 2/15/17 24 14. The representation theory of sl2(C): 2/17/17 25 15. Solvable and nilpotent Lie algebras: 2/20/17 27 16. Semisimple Lie algebras: 2/22/17 29 17. Invariant bilinear forms on Lie algebras: 2/24/17 31 18. Classical Lie groups and Lie algebras: 2/27/17 32 19. Roots and root spaces: 3/1/17 34 20. Properties of roots: 3/3/17 36 21. Root systems: 3/6/17 37 22. Dynkin diagrams: 3/8/17 39 23. -
Leonhard Euler - Wikipedia, the Free Encyclopedia Page 1 of 14
Leonhard Euler - Wikipedia, the free encyclopedia Page 1 of 14 Leonhard Euler From Wikipedia, the free encyclopedia Leonhard Euler ( German pronunciation: [l]; English Leonhard Euler approximation, "Oiler" [1] 15 April 1707 – 18 September 1783) was a pioneering Swiss mathematician and physicist. He made important discoveries in fields as diverse as infinitesimal calculus and graph theory. He also introduced much of the modern mathematical terminology and notation, particularly for mathematical analysis, such as the notion of a mathematical function.[2] He is also renowned for his work in mechanics, fluid dynamics, optics, and astronomy. Euler spent most of his adult life in St. Petersburg, Russia, and in Berlin, Prussia. He is considered to be the preeminent mathematician of the 18th century, and one of the greatest of all time. He is also one of the most prolific mathematicians ever; his collected works fill 60–80 quarto volumes. [3] A statement attributed to Pierre-Simon Laplace expresses Euler's influence on mathematics: "Read Euler, read Euler, he is our teacher in all things," which has also been translated as "Read Portrait by Emanuel Handmann 1756(?) Euler, read Euler, he is the master of us all." [4] Born 15 April 1707 Euler was featured on the sixth series of the Swiss 10- Basel, Switzerland franc banknote and on numerous Swiss, German, and Died Russian postage stamps. The asteroid 2002 Euler was 18 September 1783 (aged 76) named in his honor. He is also commemorated by the [OS: 7 September 1783] Lutheran Church on their Calendar of Saints on 24 St. Petersburg, Russia May – he was a devout Christian (and believer in Residence Prussia, Russia biblical inerrancy) who wrote apologetics and argued Switzerland [5] forcefully against the prominent atheists of his time. -
The Solution to a Generalized Toda Lattice and Representation Theory
ADVANCES IN MATHEMATICS 34,195338 (1979) The Solution to a Generalized Toda Lattice and Representation Theory BERTRAM KOSTANT* Department of Mathematics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 CONTENTS 0. Introduction 0.1. Statement of the main results 0.2. A brief description of Sections l-7 0.3. General comments 1. Poisson commutatierity of translated invariants 1.1. A formula for the Poisson bracket 1.2. The case of a subalgebra of a semi-simple Lie algebra 1.3. Relating cent 8’ to S(g)’ 1.4. The theorem [I’, Jf3 = 0 for Lie summands 1.5. The case of a Bore1 subalgebra where f = C e-,. 1.6. The commutativity of certain vector fields on a;’ 2. The variety Z of normalized Jacobi elements 2.1. The variety 8, = f + d and invariants I E So 2.2. The vector fields II, I E So, on Z 2.3. The subvarieties Z(y) Z; Z and IV-conjugacy 2.4. The Bruhat-Gelfand decomposition, the isomorphism j3,: Q* -+ Z(r), and the rationality of Z(y) in the complex case 2.5. The foliation Z = U Z(r) in the complex case 2.6. The isomorphism b(W): G1”,, + Z(y) in the complex case 3. The parametrization Z s H x A, in the real case 3.1. The polar decomposition and centralizers # 3.2. The relation Gv n RHN = G,u for y E Z and the isomorphism Z(y) z [w’ 3.3. The open Weyl chamber R, and Z 3.4. The normalizer G of 9 in Ad gc and the subset G(*) = s(K)G* C G 3.5. -
Lagrangian Mechanics - Wikipedia, the Free Encyclopedia Page 1 of 11
Lagrangian mechanics - Wikipedia, the free encyclopedia Page 1 of 11 Lagrangian mechanics From Wikipedia, the free encyclopedia Lagrangian mechanics is a re-formulation of classical mechanics that combines Classical mechanics conservation of momentum with conservation of energy. It was introduced by the French mathematician Joseph-Louis Lagrange in 1788. Newton's Second Law In Lagrangian mechanics, the trajectory of a system of particles is derived by solving History of classical mechanics · the Lagrange equations in one of two forms, either the Lagrange equations of the Timeline of classical mechanics [1] first kind , which treat constraints explicitly as extra equations, often using Branches [2][3] Lagrange multipliers; or the Lagrange equations of the second kind , which Statics · Dynamics / Kinetics · Kinematics · [1] incorporate the constraints directly by judicious choice of generalized coordinates. Applied mechanics · Celestial mechanics · [4] The fundamental lemma of the calculus of variations shows that solving the Continuum mechanics · Lagrange equations is equivalent to finding the path for which the action functional is Statistical mechanics stationary, a quantity that is the integral of the Lagrangian over time. Formulations The use of generalized coordinates may considerably simplify a system's analysis. Newtonian mechanics (Vectorial For example, consider a small frictionless bead traveling in a groove. If one is tracking the bead as a particle, calculation of the motion of the bead using Newtonian mechanics) mechanics would require solving for the time-varying constraint force required to Analytical mechanics: keep the bead in the groove. For the same problem using Lagrangian mechanics, one Lagrangian mechanics looks at the path of the groove and chooses a set of independent generalized Hamiltonian mechanics coordinates that completely characterize the possible motion of the bead. -
Math.RT] 3 Feb 2006 .Tehiebr Group Heisenberg the 8
KYUNGPOOK Math J. 42(2002), 199-272 The Method of Orbits for Real Lie Groups Jae-Hyun Yang Department of Mathematics, Inha University, Incheon 402-751, Korea e-mail : [email protected] (2000 Mathematics Subject Classification: Primary 22-XX, 20C35.) In this paper, we outline a development of the theory of orbit method for representa- tions of real Lie groups. In particular, we study the orbit method for representations of the Heisenberg group and the Jacobi group. Contents 1. Introduction 2. Quantization 3. The Kirillov Correspondence 4. Auslander-Kostant’s Theorem 5. The Obstacle for the Orbit Method 5.1. Compact Lie Groups 5.2. Semisimple Lie Groups 6. Nilpotent Orbits and the Kostant-Sekiguchi Correspondence 6.1. Jordan Decomposition 6.2. Nilpotent Orbits 6.3. The Kostant-Sekiguchi Correspondence 6.4. The Quantization of the K-action (due to D. Vogan) 7. Minimal Representations (g,h) 8. The Heisenberg Group HR 8.1. Schr¨odinger Representations 8.2. The Coadjoint Orbits of Picture 9. The Jacobi Group J arXiv:math/0602056v1 [math.RT] 3 Feb 2006 9.1. The Jacobi Group G 9.1.1. The Standard Coordinates of the Jacobi Group GJ 9.1.2. The Iwasawa Decomposition of the Jacobi Group GJ 9.2. The Lie Algebra of the Jacobi Group GJ (Received: December 4, 2001. Revised: May 14, 2002.) Key words and phrases: quantization, the Kirillov correspondence, nilpotent orbits, the Kostant-Sekiguchi correspondence, minimal representations, Heisenberg groups, the Jacobi group. This work was supported by INHA UNIVERSITY Research Grant.(INHA-21382) 199 200 Jae-Hyun Yang 9.3. -
Gravitational Edge Modes, Coadjoint Orbits, and Hydrodynamics
Gravitational Edge Modes, Coadjoint Orbits, and Hydrodynamics William Donnelly,1 Laurent Freidel,1 Seyed Faroogh Moosavian,1;2 Antony J. Speranza1 1Perimeter Institute for Theoretical Physics, 31 Caroline St. N., Waterloo ON, N2L 2Y5, Canada 2Department of Physics, McGill University, Ernest Rutherford Physics Building, 3600 Rue Univer- sity, Montr´eal, QC H3A 2T8, Canada E-mail: [email protected], [email protected], [email protected], [email protected] Abstract: The phase space of general relativity in a finite subregion is characterized by edge modes localized at the codimension-2 boundary, transforming under an infinite- dimensional group of symmetries. The quantization of this symmetry algebra is conjectured to be an important aspect of quantum gravity. As a step towards quantization, we derive a complete classification of the positive-area coadjoint orbits of this group for boundaries that are topologically a 2-sphere. This classification parallels Wigner's famous classification of representations of the Poincar´egroup since both groups have the structure of a semidirect product. We find that the total area is a Casimir of the algebra, analogous to mass in the Poincar´egroup. A further infinite family of Casimirs can be constructed from the curvature of the normal bundle of the boundary surface. These arise as invariants of the little group, which is the group of area-preserving diffeomorphisms, and are the analogues of spin. Additionally, we show that the symmetry group of hydrodynamics appears as a reduction of the corner symmetries of general relativity. Coadjoint orbits of both groups are classified by the same arXiv:2012.10367v1 [hep-th] 18 Dec 2020 set of invariants, and, in the case of the hydrodynamical group, the invariants are interpreted as the generalized enstrophies of the fluid. -
History of Mathematics in the Eighteenth Century
MATHEMATICS Craig Fraser Considered broadly, mathematical activity in the eighteenth century was characterized by a strong emphasis on analysis and mechanics. The great ad- vances occurred in the development of calculus-related parts of mathematics and in the detailed elaboration of the program of inertial mechanics founded during the Scientific Revolution. There were other mathematical develop- ments of note – in the theory of equations, number theory, probability and statistics, and geometry – but none of them reached anything like the depth and scope attained in analysis and mechanics. The close relationship between mathematics and mechanics had a basis that extended deep into Enlightenment thought. In the Preliminary Discourse to the famous French Encyclopédie, Jean d’Alembert distinguished between “pure” mathematics (geometry, arithmetic, algebra, calculus) and “mixed” mathe- matics (mechanics, geometrical astronomy, optics, art of conjecturing). He classified mathematics more generally as a “science of nature” and separated it from logic, a “science of man.” An internalized and critical spirit of inquiry, associated with the invention of new mathematical structures (for example, non-commutative algebra, non-Euclidean geometry, logic, set theory), rep- resents characteristics of modern mathematics that would emerge only in the next century. Although there were several notable British mathematicians of the period – Abraham De Moivre, James Stirling, Brook Taylor, and Colin Maclaurin among them – the major lines of mathematical production occurred on the Continent, a trend that intensified as the century developed.1 Leadership was provided by a relatively small number of energetic figures: Jakob, Johann, and Daniel Bernoulli, Jakob Hermann, Leonhard Euler, Alexis Clairaut, Jean d’Alembert, Johann Heinrich Lambert, Joseph Louis Lagrange, Adrien Marie Legendre, and Pierre Simon Laplace. -
The 18Th-Century Battle Over Lunar Motion - Physics Today Janu
The 18th-century battle over lunar motion - Physics Today Janu... http://ptonline.aip.org/servlet/PrintPTJ Physics Today URL: http://ptonline.aip.org/journals/doc/PHTOAD-ft/vol_63/iss_1 Published: January 2010 /27_1.shtml [Permission to reprint or copy this article/photo must be obtained from Physics Today. Call 301-209-3042 or e-mail [email protected] with your request.] ARTICLES The 18th-century battle over lunar motion In a dispute with more than just scientific import, Alexis Clairaut, Leonhard Euler, and Jean le Rond d’Alembert each employed their own strategies to establish that they were the first to understand a puzzling feature of the Moon’s orbit. Siegfried Bodenmann About two years after Sputnik 1 began emitting radio signals, the Soviet Union’s Luna 2 became the first manmade object to reach the Moon. The intentional crash landing of the spacecraft on 13 September 1959 once again demonstrated Soviet technological superiority over the US. That event can be regarded as the trigger of the so-called race to the Moon, initiated by President John F. Kennedy in May 1961. As the much-broadcast commemoration of Apollo 11 and the first manned landing on the Moon reminded us, the Americans won the competition. Every story has a prologue. The one preceding Neil Armstrong’s historic steps shows that a captivating plot from the past needn’t include a cold war or spies. It tells of three men who competed to develop a predictive theory that would accurately describe the motion of the Moon and therefore furnish a key tool that, much later, would help the Soviets and the Americans anticipate the position of their celestial target.