Type II hidden symmetries of the Laplace equation
|
|
- Leslie Harvey
- 5 years ago
- Views:
Transcription
1 Type II hidden symmetries of the Laplace equation Andronikos Paliathanasis Larnaka, 2014 A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
2 Plan of the Talk 1 The generic symmetry vector of second order PDE s 2 De nition of Type II hidden symmetries 3 Reduction of the Laplace equation in Riemannian spaces and the origin of Type II hidden symmetries 4 Applications A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
3 Lie symmetries of a general second order PDE Lie symmetry conditions Consider the second order PDE H : A ij x k, u u ij B k (x, u)u k f (x, u) = 0. where A ij is a non degenerate tensor and X = ξ i x k, u i + η x k, u u is the generator of a in nitesimal transformation. We shall say that the vector eld X will be a Lie symmetry of the PDE H if there exist a function λ such as X [2] H = λh where X [2] is the second prologation vector of X. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
4 Lie symmetries of a general second order PDE Lie symmetry conditions From the Lie symmetry condition we have the following determining system A ij (a ij u + b ij ) (a,i u + b,i )B i ξ k f,k auf,u bf,u + λf = 0 A ij ξ k,ij 2A ik a,i + ab k + aub k,u ξ k,i Bi + ξ i B k,i λb k + bb k,u = 0 L X A ij = (λ a)a ij (1) η = a(x i )u + b(x i ), ξ k,u = 0, ξk (x i ). Eq. (1) implies that the symmetry vector X is a CKV of the second order tensor A ij. with conformal factor ψ = 1 2 (a λ). A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
5 Lie symmetries Poisson equation Theorem The Lie symmetries of the Poisson equation u f x i, u = 0, = p 1 pjgjg ij are generated from the jg j x i x j CKVs of the metric g ij de ning the Laplace operator. The generic Lie symmetry vector is 2 n X = ξ i x k i + ψ x k u + a 0 u + b x k u 2 where ξ i x k is a CKV with conformal factor ψ x k and the following condition holds 2 n 2 ψu + g ij b i;j ξ k 2 n f,k ψuf,u n ψf bf,u = 0. (2) 2 A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
6 Lie symmetries Laplace equations In the case of the Laplace equation u = 0, the symmetry condition becomes 2 n 2 ψ = 0. That means that if n > 2 the CKVs generate a Lie point symmetry for the Laplace equation if and only if the conformal factor ψ x k satis es the Laplace equation. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
7 Type II hidden Symmetries De nition Consider an ODE which admits the Lie point symmetries X 1, X 2 which are such that [X 1, X 2 ] = C12 1 X 1. Then, the reduction by X 1 leads to a reduced equation which admits X 2 as a Lie symmetry whereas reduction of the ODE by X 2 leads to a reduced equation, which does not admit X 1 as a Lie symmetry. In case the generators X 1, X 2 form an Abelian Lie algebra, i.e. [X 1, X 2 ] = 0, then, the reduction preserves the Lie symmetries. Since the reduced equation is di erent from the original equation, it is possible the reduced equation to admit extra Lie symmetries, which are not Lie symmetries of the original equation. These new Lie symmetries have been named Type II hidden symmetries. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
8 Type II hidden Symmetries Problem Study the origin of Type II hidden symmetries of the Laplace equation in certain Riemannian spaces A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
9 Laplace eqn. in Riemannian spaces In a general Riemannian space, Laplace eqn. u = 0, admits the Lie symmetries X u = u u, X b = b (t, x) u where b (t, x) is a solution of Laplace equation and X u existed since the Laplace eqn. is linear. We restrict our considerations to spaces which admit a conformal algebra (proper or not) in order to have extra Lie symmetries and to apply the zero order invariants to reduce the Laplace eqn. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
10 Laplace eqn. in Riemannian spaces a. If a (1 + n) d R.s. admits a gradient KV, the S i = z the metric is ds 2 = dz 2 + h AB y A y B, h AB = h AB y C b. If a (1 + n) d R.s. admits a gradient HV, the H i = r r the metric is ds 2 = dr 2 + r 2 h AB dy A dy B, h AB = h AB y C c. If a (1 + n) d R.s. admits a sp.ckv then admits a gradient KV and a gradient HV and the metric can be written in the generic form ds 2 = dz 2 + dr 2 + R 2 f AB y C dy A dy B while the sp.ckv is C S = z 2 +R 2 2 z + zr R with conformal factor ψ CS = z. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
11 Reduction with a gr. KV The Laplace equation in a Riemannian space which admit the gr. KV z can be written as follows u zz + h AB y C u AB Γ A y C u B = 0. (3) The Laplace equation admits as extra Lie symmetry the gradient KV z. By using the zeroth order invariants y A, w = u of z the reduced equation is h w = 0. We recall the following geometrical results A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
12 Reduction with a gr. KV The KVs of the n metric are identical with those of the n + 1 metric The 1 + n metric admits a HV if and only if the n metric admits one and if n H A is the HV of the n metric then the HV of the 1 + n metric is given by the expression 1+nH µ = zδ µ z + n H A δ µ A µ = x, 1,..., n. (4) The 1 + n metric admits CKVs if and only if the n metric h AB admits a gradient CKV. Therefore Type II hidden symmetries exist if the n metric h AB admits more symmetries. Speci cally, the sp.ckvs of the h AB metric as well as the proper CKVs whose conformal function is a solution of Laplace equation generate Type II hidden symmetries. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
13 Reduction with a gr. HV In Riemannian spaces which admit a gradient HV, H = r r, the Laplace equation becomes u rr + 1 r 2 hab y C u AB + (n 1) 1 u r r r 2 ΓA y C u A = 0 (5) and admits the extra Lie symmetry H. The zeroth order invariants of H are y A, w y A and using them it follows easily that the reduced equation is h u = 0 (6) that is, the Laplacian de ned by the metric h AB. It is easy to establish the following results concerning the conformal algebras of the metrics g ij and h AB. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
14 Reduction with a gr. HV The KVs of h AB are also KVs of g ij. The HV of g ij is independent from that of h AB. The metric g ij admits proper CKVs if and only if the n metric h AB admits gradient CKVs. This is because g ij is conformally related with the decomposable metric ds 20 = dr 2 + h AB y C dy A dy B. (7) The above imply, that Type II hidden symmetries we shall have from the HV of the metric h AB, the sp.ckvs and nally from the proper CKVs of h AB whose conformal factor is a solution of Laplace equation h u = 0. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
15 Reduction with a sp.ckv In a Riemannian space which admit a sp. CKV the Laplace equation is u zz + u RR + 1 R 2 hab u AB + and admits the Lie point symmetries where 2p = 1 m (m 1) 1 u R R R 2 ΓA u A = 0. (8) X 1 = K G, X 2 = H, X 3 = C S + 2pzu u 2 and the non zero commutators are X 1, X 2 = X 1, X 2, X 3 = X 3 X 1, X 3 = X 2 + 2pX u. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
16 Reduction with a sp.ckv Under the coordinate transformation z = q R (xr 1) x invariants of the Lie symmetry X 3 are x, y A, w = ur 2p. The reduced equation is the zero order x 2 w xx + f AB w AB Γ A w A 2p (2p + 1) w = 0 If dim (f AB ) = 2, the reduced equation becomes (m=3) w = 0 which is the Laplacian in the three dimensional space with metric d s 2 (m=3) = 1 x 4 dx2 + 1 x 2 f AB dy A dy B. (9) By making the new transformation x = 1 r, the metric admits the gradient HV r r which gives an inherited symmetry. We conclude that Type II hidden symmetries of (9) will be generated from the proper CKVs of the metric (9). A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
17 Reduction with a sp.ckv If dim (f AB ) 3, if we apply the transformation x = (m 2) 2 m φ m 2 the reduced equation becomes where V (x) = V (φ) = (m4) w 2p (2p + 1) V (φ) w = 0 (10) (2 m)2 φ 2 (m4) is the Laplace operator with metric is the well known Ermakov potential and d s 2 (m4) = dφ2 + φ 2 f AB dy A dy B (11) The reduced equation is a KG equation. It is easy to see that the gradient HV φ φ of (11) is a Lie symmetry of (??) which is the Lie symmetry X 2. Therefore, if the metric f AB admits proper CKVs then these vectors generate Type II hidden symmetries. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
18 Type II hidden Symmetries Laplace equation: Main Results If we reduce the Laplace equation with a gradient KV the reduced equation is a Laplace equation in the non-decomposable space. In this case, the Type II hidden symmetries are generated from the special and the proper CKVs of the non-decomposable space. If we reduce the Laplace equation with a gradient HV the reduced equation is a Laplace equation for an appropriate metric. In this case, the Type II hidden symmetries are generated from the HV and the special/proper CKVs. If we reduce the Laplace equation with the symmetry generated by a sp.ckv, the reduced equation is the Klein Gordon equation for an appropriate metric that inherits the Lie point symmetry generated by the gradient HV. In this case, the Type II hidden symmetries are generated from the proper CKVs of the appropriate metric. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
19 1+3 Wave equation Consider the Laplace equation in the four dimensional Minkowski spacetime M 4 u tt u xx u yy u zz = 0. The Lie point symmetries are: K 1 G, K A G, X 1A R, X AB R, H, X 1 C tu u, X A C y A u u where y A = (x, y, z). The nonzero commutators are h i h i i KG I, X R IJ = KG J, KG I, H = KG hk I, G I, X C I = H X u h i i h i KG I, X C J = XR hh, IJ, XC I = XC I, XR IJ, X C I = XC J. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
20 1+3 Wave equation Reduction with a gr. KV Reduction with the gradient KV K z G = z. The reduced equation is w tt w xx w yy = 0 which is Laplace equation in the space M 3. The Lie symmetries are KG 1, K G x, K y G, X C tu u, X C x X 1a R, XR ab (12) 1 2 yu u (13) 1 2 xu u, X y C K, X R, H are inherited symmetries the other vectors are Type II hidden symmetries which are generated from the sp.ckvs of M 3. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
21 1+3 Wave equation Reduction with a gr HV In spherical coordinates the HV is H = r r. The reduced equation is w θθ + w φφ cosh 2 θ + w ζζ cosh 2 θ cosh φ 2 + 2tanh θ r 2 w θ + tanh φ r 2 cosh 2 θ w φ = 0. which is the Laplace in a space of constant curvature. The Lie symmetries of the reduced equation are the elements of the so (3) Lie algebra and are inherits symmetries. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
22 Type II hidden Symmetries Reduction with a sp.ckv In the reduction with a sp.ckv we found that the reduce equation is the 3d Laplace equation in M 3. The M 3 does not admits proper (non special) CKVs here there are not any type II hidden symmetries. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
23 1+2 Wave equation The wave equation in E 2 is u tt u xx u yy = 0. (14) Reduction with the gradient KV K y G = y. The reduced equation is w tt w xx which is the one dimensional wave equation. The 2d space (t, x) has an in nite number of CKVs therefore the reduced equations has in nite Lie point symmetries. From these symmetries the KVs and the HV are inherited symmetries and the CKVs are Type II symmetries. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
24 1+2 Wave equation In order to do the reduction with the gradient HV we introduce spherical coordinates (r, θ, φ). The Laplace equation is 1 u rr r 2 u θθ + u φφ cosh θ r u r tanh θ r 2 u θ = 0. (15) Therefore by applying the zero order invariants of the HV the reduced equation is w θθ + w φφ cosh 2 θ + tanh θw θ = 0. (16) By making the transformation θ = ln tan ρ 2 equation (16) becomes sin (x) 2 w ρρ + w φφ = 0 which is the wave equation (??) with t = ρ, x = iφ. A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
25 Conclusion Thank you! A. Paliathanasis (Univ. of Naples) Type II symmetries Larnaka, / 25
General Relativity I
General Relativity I presented by John T. Whelan The University of Texas at Brownsville whelan@phys.utb.edu LIGO Livingston SURF Lecture 2002 July 5 General Relativity Lectures I. Today (JTW): Special
More informationMathematical Journal of Okayama University
Mathematical Journal of Okayama University Volume 42 Issue 2000 Article 6 JANUARY 2000 Certain Metrics on R 4 + Tominosuke Otsuki Copyright c 2000 by the authors. Mathematical Journal of Okayama University
More informationExact Solutions of the Einstein Equations
Notes from phz 6607, Special and General Relativity University of Florida, Fall 2004, Detweiler Exact Solutions of the Einstein Equations These notes are not a substitute in any manner for class lectures.
More informationSpacetime and 4 vectors
Spacetime and 4 vectors 1 Minkowski space = 4 dimensional spacetime Euclidean 4 space Each point in Minkowski space is an event. In SR, Minkowski space is an absolute structure (like space in Newtonian
More informationChapter 4. The First Fundamental Form (Induced Metric)
Chapter 4. The First Fundamental Form (Induced Metric) We begin with some definitions from linear algebra. Def. Let V be a vector space (over IR). A bilinear form on V is a map of the form B : V V IR which
More informationChapter 3. Second Order Linear PDEs
Chapter 3. Second Order Linear PDEs 3.1 Introduction The general class of second order linear PDEs are of the form: ax, y)u xx + bx, y)u xy + cx, y)u yy + dx, y)u x + ex, y)u y + f x, y)u = gx, y). 3.1)
More information9 Symmetries of AdS 3
9 Symmetries of AdS 3 This section consists entirely of exercises. If you are not doing the exercises, then read through them anyway, since this material will be used later in the course. The main goal
More informationWarped Products. by Peter Petersen. We shall de ne as few concepts as possible. A tangent vector always has the local coordinate expansion
Warped Products by Peter Petersen De nitions We shall de ne as few concepts as possible. A tangent vector always has the local coordinate expansion a function the di erential v = dx i (v) df = f dxi We
More information4.3 - Linear Combinations and Independence of Vectors
- Linear Combinations and Independence of Vectors De nitions, Theorems, and Examples De nition 1 A vector v in a vector space V is called a linear combination of the vectors u 1, u,,u k in V if v can be
More informationVectors. Three dimensions. (a) Cartesian coordinates ds is the distance from x to x + dx. ds 2 = dx 2 + dy 2 + dz 2 = g ij dx i dx j (1)
Vectors (Dated: September017 I. TENSORS Three dimensions (a Cartesian coordinates ds is the distance from x to x + dx ds dx + dy + dz g ij dx i dx j (1 Here dx 1 dx, dx dy, dx 3 dz, and tensor g ij is
More informationSpherical Coordinates and Legendre Functions
Spherical Coordinates and Legendre Functions Spherical coordinates Let s adopt the notation for spherical coordinates that is standard in physics: φ = longitude or azimuth, θ = colatitude ( π 2 latitude)
More informationMATH 131P: PRACTICE FINAL SOLUTIONS DECEMBER 12, 2012
MATH 3P: PRACTICE FINAL SOLUTIONS DECEMBER, This is a closed ook, closed notes, no calculators/computers exam. There are 6 prolems. Write your solutions to Prolems -3 in lue ook #, and your solutions to
More informationConformal Killing Vectors in LRS Bianchi Type V Spacetimes
Commun. Theor. Phys. 65 (016 315 30 Vol. 65, No. 3, March 1, 016 Conformal Killing Vectors in LRS Bianchi Type V Spacetimes Suhail Khan, 1 Tahir Hussain, 1, Ashfaque H. Bokhari, and Gulzar Ali Khan 1 1
More informationFinal Exam May 4, 2016
1 Math 425 / AMCS 525 Dr. DeTurck Final Exam May 4, 2016 You may use your book and notes on this exam. Show your work in the exam book. Work only the problems that correspond to the section that you prepared.
More informationCLASSIFICATION AND PRINCIPLE OF SUPERPOSITION FOR SECOND ORDER LINEAR PDE
CLASSIFICATION AND PRINCIPLE OF SUPERPOSITION FOR SECOND ORDER LINEAR PDE 1. Linear Partial Differential Equations A partial differential equation (PDE) is an equation, for an unknown function u, that
More informationBessel s Equation. MATH 365 Ordinary Differential Equations. J. Robert Buchanan. Fall Department of Mathematics
Bessel s Equation MATH 365 Ordinary Differential Equations J. Robert Buchanan Department of Mathematics Fall 2018 Background Bessel s equation of order ν has the form where ν is a constant. x 2 y + xy
More informationKonstantin E. Osetrin. Tomsk State Pedagogical University
Space-time models with dust and cosmological constant, that allow integrating the Hamilton-Jacobi test particle equation by separation of variables method. Konstantin E. Osetrin Tomsk State Pedagogical
More informationUNIVERSITY OF DUBLIN
UNIVERSITY OF DUBLIN TRINITY COLLEGE JS & SS Mathematics SS Theoretical Physics SS TSM Mathematics Faculty of Engineering, Mathematics and Science school of mathematics Trinity Term 2015 Module MA3429
More informationHomework 3 solutions Math 136 Gyu Eun Lee 2016 April 15. R = b a
Homework 3 solutions Math 136 Gyu Eun Lee 2016 April 15 A problem may have more than one valid method of solution. Here we present just one. Arbitrary functions are assumed to have whatever regularity
More informationSalmon: Lectures on partial differential equations
6. The wave equation Of the 3 basic equations derived in the previous section, we have already discussed the heat equation, (1) θ t = κθ xx + Q( x,t). In this section we discuss the wave equation, () θ
More informationMath 4263 Homework Set 1
Homework Set 1 1. Solve the following PDE/BVP 2. Solve the following PDE/BVP 2u t + 3u x = 0 u (x, 0) = sin (x) u x + e x u y = 0 u (0, y) = y 2 3. (a) Find the curves γ : t (x (t), y (t)) such that that
More informationAero III/IV Conformal Mapping
Aero III/IV Conformal Mapping View complex function as a mapping Unlike a real function, a complex function w = f(z) cannot be represented by a curve. Instead it is useful to view it as a mapping. Write
More informationTeleparallel Lie Symmetries of FRW Spacetime by Using Diagonal Tetrad
J. Appl. Environ. Biol. Sci., (7S)-9,, TextRoad Publication ISSN: 9-7 Journal of Applied Environmental and Biological Sciences www.textroad.com Teleparallel Lie Symmetries of FRW Spacetime by Using Diagonal
More informationSymmetry Reductions of (2+1) dimensional Equal Width. Wave Equation
Authors: Symmetry Reductions of (2+1) dimensional Equal Width 1. Dr. S. Padmasekaran Wave Equation Asst. Professor, Department of Mathematics Periyar University, Salem 2. M.G. RANI Periyar University,
More informationErrata for Robot Vision
Errata for Robot Vision This is a list of known nontrivial bugs in Robot Vision 1986 by B.K.P. Horn, MIT Press, Cambridge, MA ISBN 0-262-08159-8 and McGraw-Hill, New York, NY ISBN 0-07-030349-5. If you
More informationAlgorithmic Lie Symmetry Analysis and Group Classication for Ordinary Dierential Equations
dmitry.lyakhov@kaust.edu.sa Symbolic Computations May 4, 2018 1 / 25 Algorithmic Lie Symmetry Analysis and Group Classication for Ordinary Dierential Equations Dmitry A. Lyakhov 1 1 Computational Sciences
More informationKerr black hole and rotating wormhole
Kerr Fest (Christchurch, August 26-28, 2004) Kerr black hole and rotating wormhole Sung-Won Kim(Ewha Womans Univ.) August 27, 2004 INTRODUCTION STATIC WORMHOLE ROTATING WORMHOLE KERR METRIC SUMMARY AND
More informationNotes 19 Gradient and Laplacian
ECE 3318 Applied Electricity and Magnetism Spring 218 Prof. David R. Jackson Dept. of ECE Notes 19 Gradient and Laplacian 1 Gradient Φ ( x, y, z) =scalar function Φ Φ Φ grad Φ xˆ + yˆ + zˆ x y z We can
More informationVariable separation and second order superintegrability
Variable separation and second order superintegrability Willard Miller (Joint with E.G.Kalnins) miller@ima.umn.edu University of Minnesota IMA Talk p.1/59 Abstract In this talk we shall first describe
More informationBrief course of lectures at 18th APCTP Winter School on Fundamental Physics
Brief course of lectures at 18th APCTP Winter School on Fundamental Physics Pohang, January 20 -- January 28, 2014 Motivations : (1) Extra-dimensions and string theory (2) Brane-world models (3) Black
More informationGeneral Relativity (225A) Fall 2013 Assignment 8 Solutions
University of California at San Diego Department of Physics Prof. John McGreevy General Relativity (5A) Fall 013 Assignment 8 Solutions Posted November 13, 013 Due Monday, December, 013 In the first two
More informationSINGULAR CURVES OF AFFINE MAXIMAL MAPS
Fundamental Journal of Mathematics and Mathematical Sciences Vol. 1, Issue 1, 014, Pages 57-68 This paper is available online at http://www.frdint.com/ Published online November 9, 014 SINGULAR CURVES
More informationUNIVERSITY of LIMERICK OLLSCOIL LUIMNIGH
UNIVERSITY of LIMERICK OLLSCOIL LUIMNIGH Faculty of Science and Engineering Department of Mathematics and Statistics END OF SEMESTER ASSESSMENT PAPER MODULE CODE: MA4006 SEMESTER: Spring 2011 MODULE TITLE:
More informationSymmetry analysis of the cylindrical Laplace equation
Symmetry analysis of the cylindrical Laplace equation Mehdi Nadjafikhah Seyed-Reza Hejazi Abstract. The symmetry analysis for Laplace equation on cylinder is considered. Symmetry algebra the structure
More informationPhysics/Astronomy 226, Problem set 4, Due 2/10 Solutions. Solution: Our vectors consist of components and basis vectors:
Physics/Astronomy 226, Problem set 4, Due 2/10 Solutions Reading: Carroll, Ch. 3 1. Derive the explicit expression for the components of the commutator (a.k.a. Lie bracket): [X, Y ] u = X λ λ Y µ Y λ λ
More informationIntroduction to Group Theory
Introduction to Group Theory Ling-Fong Li (Institute) Group 1 / 6 INTRODUCTION Group theory : framework for studying symmetry. The representation theory of the group simpli es the physical solutions. For
More informationQuantum Mechanics in Three Dimensions
Physics 342 Lecture 21 Quantum Mechanics in Three Dimensions Lecture 21 Physics 342 Quantum Mechanics I Monday, March 22nd, 21 We are used to the temporal separation that gives, for example, the timeindependent
More informationComplete integrability of geodesic motion in Sasaki-Einstein toric spaces
Complete integrability of geodesic motion in Sasaki-Einstein toric spaces Mihai Visinescu Department of Theoretical Physics National Institute for Physics and Nuclear Engineering Horia Hulubei Bucharest,
More informationUniformity of the Universe
Outline Universe is homogenous and isotropic Spacetime metrics Friedmann-Walker-Robertson metric Number of numbers needed to specify a physical quantity. Energy-momentum tensor Energy-momentum tensor of
More informationLiouville integrability of Hamiltonian systems and spacetime symmetry
Seminar, Kobe U., April 22, 2015 Liouville integrability of Hamiltonian systems and spacetime symmetry Tsuyoshi Houri with D. Kubiznak (Perimeter Inst.), C. Warnick (Warwick U.) Y. Yasui (OCU Setsunan
More informationThe Klein-Gordon Equation Meets the Cauchy Horizon
Enrico Fermi Institute and Department of Physics University of Chicago University of Mississippi May 10, 2005 Relativistic Wave Equations At the present time, our best theory for describing nature is Quantum
More informationMinkowski spacetime. Pham A. Quang. Abstract: In this talk we review the Minkowski spacetime which is the spacetime of Special Relativity.
Minkowski spacetime Pham A. Quang Abstract: In this talk we review the Minkowski spacetime which is the spacetime of Special Relativity. Contents 1 Introduction 1 2 Minkowski spacetime 2 3 Lorentz transformations
More informationAn Introduction to Kaluza-Klein Theory
An Introduction to Kaluza-Klein Theory A. Garrett Lisi nd March Department of Physics, University of California San Diego, La Jolla, CA 993-39 gar@lisi.com Introduction It is the aim of Kaluza-Klein theory
More informationMulti-disformal invariance of nonlinear primordial perturbations
Multi-disformal invariance of nonlinear primordial perturbations Yuki Watanabe Natl. Inst. Tech., Gunma Coll.) with Atsushi Naruko and Misao Sasaki accepted in EPL [arxiv:1504.00672] 2nd RESCEU-APCosPA
More informationÜbungen zu RT2 SS (4) Show that (any) contraction of a (p, q) - tensor results in a (p 1, q 1) - tensor.
Übungen zu RT2 SS 2010 (1) Show that the tensor field g µν (x) = η µν is invariant under Poincaré transformations, i.e. x µ x µ = L µ νx ν + c µ, where L µ ν is a constant matrix subject to L µ ρl ν ση
More informationResearch Article Equivalent Lagrangians: Generalization, Transformation Maps, and Applications
Journal of Applied Mathematics Volume 01, Article ID 86048, 19 pages doi:10.1155/01/86048 Research Article Equivalent Lagrangians: Generalization, Transformation Maps, and Applications N. Wilson and A.
More informationProblem 1, Lorentz transformations of electric and magnetic
Problem 1, Lorentz transformations of electric and magnetic fields We have that where, F µν = F µ ν = L µ µ Lν ν F µν, 0 B 3 B 2 ie 1 B 3 0 B 1 ie 2 B 2 B 1 0 ie 3 ie 2 ie 2 ie 3 0. Note that we use the
More informationν(u, v) = N(u, v) G(r(u, v)) E r(u,v) 3.
5. The Gauss Curvature Beyond doubt, the notion of Gauss curvature is of paramount importance in differential geometry. Recall two lessons we have learned so far about this notion: first, the presence
More informationFinal: Solutions Math 118A, Fall 2013
Final: Solutions Math 118A, Fall 2013 1. [20 pts] For each of the following PDEs for u(x, y), give their order and say if they are nonlinear or linear. If they are linear, say if they are homogeneous or
More informationDerivatives in General Relativity
Derivatives in General Relativity One of the problems with curved space is in dealing with vectors how do you add a vector at one point in the surface of a sphere to a vector at a different point, and
More informationInvariant Nonholonomic Riemannian Structures on Three-Dimensional Lie Groups
Invariant Nonholonomic Riemannian Structures on Three-Dimensional Lie Groups Dennis I. Barrett Geometry, Graphs and Control (GGC) Research Group Department of Mathematics, Rhodes University Grahamstown,
More informationarxiv: v1 [math-ph] 31 Jan 2015
Symmetry, Integrability and Geometry: Methods and Applications SIGMA? (00?), 00?,?? pages Structure relations and Darboux contractions for D nd order superintegrable systems R. Heinonen, E. G. Kalnins,
More informationSpotlight on Laplace s Equation
16 Spotlight on Laplace s Equation Reference: Sections 1.1,1.2, and 1.5. Laplace s equation is the undriven, linear, second-order PDE 2 u = (1) We defined diffusivity on page 587. where 2 is the Laplacian
More informationDiscrete Differential Geometry. Discrete Laplace-Beltrami operator and discrete conformal mappings.
Discrete differential geometry. Discrete Laplace-Beltrami operator and discrete conformal mappings. Technische Universität Berlin Geometric Methods in Classical and Quantum Lattice Systems, Caputh, September
More informationGroup Classification and Similarity Solutions. of Klein Gordon Equations on a Sphere
Group Classification and Similarity Solutions of Klein Gordon Equations on a Sphere By KHALID ALI AYED AL-ANEZY May 01 This thesis is dedicated to my parents For their endless love, support and encouragement
More informationConserved Quantities in Lemaître-Tolman-Bondi Cosmology
1/15 Section 1 Section 2 Section 3 Conserved Quantities in Lemaître-Tolman-Bondi Cosmology Alex Leithes - Blackboard Talk Outline ζ SMTP Evolution Equation: ζ SMTP = H X + 2H Y 3 ρ Valid on all scales.
More informationExpansion of 1/r potential in Legendre polynomials
Expansion of 1/r potential in Legendre polynomials In electrostatics and gravitation, we see scalar potentials of the form V = K d Take d = R r = R 2 2Rr cos θ + r 2 = R 1 2 r R cos θ + r R )2 Use h =
More informationStarting from Heat Equation
Department of Applied Mathematics National Chiao Tung University Hsin-Chu 30010, TAIWAN 20th August 2009 Analytical Theory of Heat The differential equations of the propagation of heat express the most
More informationIntroduction and Vectors Lecture 1
1 Introduction Introduction and Vectors Lecture 1 This is a course on classical Electromagnetism. It is the foundation for more advanced courses in modern physics. All physics of the modern era, from quantum
More informationMathematical Tripos Part IA Lent Term Example Sheet 1. Calculate its tangent vector dr/du at each point and hence find its total length.
Mathematical Tripos Part IA Lent Term 205 ector Calculus Prof B C Allanach Example Sheet Sketch the curve in the plane given parametrically by r(u) = ( x(u), y(u) ) = ( a cos 3 u, a sin 3 u ) with 0 u
More informationHigher dimensional Kerr-Schild spacetimes 1
Higher dimensional Kerr-Schild spacetimes 1 Marcello Ortaggio Institute of Mathematics Academy of Sciences of the Czech Republic Bremen August 2008 1 Joint work with V. Pravda and A. Pravdová, arxiv:0808.2165
More informationFaculty of Engineering, Mathematics and Science School of Mathematics
Faculty of Engineering, Mathematics and Science School of Mathematics JS & SS Mathematics SS Theoretical Physics SS TSM Mathematics Module MA3429: Differential Geometry I Trinity Term 2018???, May??? SPORTS
More informationErrata for Robot Vision
Errata for Robot Vision This is a list of known nontrivial bugs in Robot Vision 1986) by B.K.P. Horn, MIT Press, Cambridge, MA ISBN 0-6-08159-8 and McGraw-Hill, New York, NY ISBN 0-07-030349-5. If you
More informationChapter 3 Second Order Linear Equations
Partial Differential Equations (Math 3303) A Ë@ Õæ Aë áöß @. X. @ 2015-2014 ú GA JË@ É Ë@ Chapter 3 Second Order Linear Equations Second-order partial differential equations for an known function u(x,
More informationHyperbolic Geometric Flow
Hyperbolic Geometric Flow Kefeng Liu CMS and UCLA August 20, 2007, Dong Conference Page 1 of 51 Outline: Joint works with D. Kong and W. Dai Motivation Hyperbolic geometric flow Local existence and nonlinear
More informationAddendum: Symmetries of the. energy-momentum tensor
Addendum: Symmetries of the arxiv:gr-qc/0410136v1 28 Oct 2004 energy-momentum tensor M. Sharif Department of Mathematics, University of the Punjab, Quaid-e-Azam Campus Lahore-54590, PAKISTAN. Abstract
More informationTutorial Exercises: Geometric Connections
Tutorial Exercises: Geometric Connections 1. Geodesics in the Isotropic Mercator Projection When the surface of the globe is projected onto a flat map some aspects of the map are inevitably distorted.
More informationFORMULA SHEET FOR QUIZ 2 Exam Date: November 8, 2017
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.07: Electromagnetism II November 5, 207 Prof. Alan Guth FORMULA SHEET FOR QUIZ 2 Exam Date: November 8, 207 A few items below are marked
More information1 A complete Fourier series solution
Math 128 Notes 13 In this last set of notes I will try to tie up some loose ends. 1 A complete Fourier series solution First here is an example of the full solution of a pde by Fourier series. Consider
More information2 General Relativity. 2.1 Curved 2D and 3D space
22 2 General Relativity The general theory of relativity (Einstein 1915) is the theory of gravity. General relativity ( Einstein s theory ) replaced the previous theory of gravity, Newton s theory. The
More informationSophus Lie s Approach to Differential Equations
Sophus Lie s Approach to Differential Equations IAP lecture 2006 (S. Helgason) 1 Groups Let X be a set. A one-to-one mapping ϕ of X onto X is called a bijection. Let B(X) denote the set of all bijections
More informationChristoffel Symbols. 1 In General Topologies. Joshua Albert. September 28, W. First we say W : λ n = x µ (λ) so that the world
Christoffel Symbols Joshua Albert September 28, 22 In General Topoloies We have a metric tensor nm defined by, Note by some handy theorem that for almost any continuous function F (L), equation 2 still
More informationWARPED PRODUCTS PETER PETERSEN
WARPED PRODUCTS PETER PETERSEN. Definitions We shall define as few concepts as possible. A tangent vector always has the local coordinate expansion v dx i (v) and a function the differential df f dxi We
More informationLecturer: Bengt E W Nilsson
9 3 19 Lecturer: Bengt E W Nilsson Last time: Relativistic physics in any dimension. Light-cone coordinates, light-cone stuff. Extra dimensions compact extra dimensions (here we talked about fundamental
More informationDraft version September 15, 2015
Novi Sad J. Math. Vol. XX, No. Y, 0ZZ,??-?? ON NEARLY QUASI-EINSTEIN WARPED PRODUCTS 1 Buddhadev Pal and Arindam Bhattacharyya 3 Abstract. We study nearly quasi-einstein warped product manifolds for arbitrary
More informationEE 333 Electricity and Magnetism, Fall 2009 Homework #9 solution
EE 333 Electricity and Magnetism, Fall 009 Homework #9 solution 4.10. The two infinite conducting cones θ = θ 1, and θ = θ are maintained at the two potentials Φ 1 = 100, and Φ = 0, respectively, as shown
More informationMATH H53 : Final exam
MATH H53 : Final exam 11 May, 18 Name: You have 18 minutes to answer the questions. Use of calculators or any electronic items is not permitted. Answer the questions in the space provided. If you run out
More informationMetrisability of Painleve equations and Hamiltonian systems of hydrodynamic type
Metrisability of Painleve equations and Hamiltonian systems of hydrodynamic type Felipe Contatto Department of Applied Mathematics and Theoretical Physics University of Cambridge felipe.contatto@damtp.cam.ac.uk
More informationTensors - Lecture 4. cos(β) sin(β) sin(β) cos(β) 0
1 Introduction Tensors - Lecture 4 The concept of a tensor is derived from considering the properties of a function under a transformation of the corrdinate system. As previously discussed, such transformations
More informationD Tangent Surfaces of Timelike Biharmonic D Helices according to Darboux Frame on Non-degenerate Timelike Surfaces in the Lorentzian Heisenberg GroupH
Bol. Soc. Paran. Mat. (3s.) v. 32 1 (2014): 35 42. c SPM ISSN-2175-1188 on line ISSN-00378712 in press SPM: www.spm.uem.br/bspm doi:10.5269/bspm.v32i1.19035 D Tangent Surfaces of Timelike Biharmonic D
More informationSymmetry Preserving Numerical Methods via Moving Frames
Symmetry Preserving Numerical Methods via Moving Frames Peter J. Olver University of Minnesota http://www.math.umn.edu/ olver = Pilwon Kim, Martin Welk Cambridge, June, 2007 Symmetry Preserving Numerical
More informationClifford Algebras and Spin Groups
Clifford Algebras and Spin Groups Math G4344, Spring 2012 We ll now turn from the general theory to examine a specific class class of groups: the orthogonal groups. Recall that O(n, R) is the group of
More informationElio Sacco. Dipartimento di Ingegneria Civile e Meccanica Università di Cassino e LM
Elio Sacco Dipartimento di Ingegneria Civile e Meccanica Università di Cassino e LM The no-tension material model is adopted to evaluate the collapse load. y Thrust curve of the arch extrados intrados
More informationSolutions to Homework from Maldacena
Solutions to Homework from Maldacena by Jolyon Bloomfield July 3, 011 1 Problem #4 We want to evaluate the action S E = R AdS 16πG N for the Euclidean AdS metric d 4 x g(r + 6) d 3 x ] hk Σ 4 Σ 4 (1) The
More informationUNIVERSITY OF MANITOBA
Question Points Score INSTRUCTIONS TO STUDENTS: This is a 6 hour examination. No extra time will be given. No texts, notes, or other aids are permitted. There are no calculators, cellphones or electronic
More information(1) Recap of Differential Calculus and Integral Calculus (2) Preview of Calculus in three dimensional space (3) Tools for Calculus 3
Math 127 Introduction and Review (1) Recap of Differential Calculus and Integral Calculus (2) Preview of Calculus in three dimensional space (3) Tools for Calculus 3 MATH 127 Introduction to Calculus III
More informationarxiv: v2 [gr-qc] 7 Jan 2019
Classical Double Copy: Kerr-Schild-Kundt metrics from Yang-Mills Theory arxiv:1810.03411v2 [gr-qc] 7 Jan 2019 Metin Gürses 1, and Bayram Tekin 2, 1 Department of Mathematics, Faculty of Sciences Bilkent
More informationMath 413/513 Chapter 6 (from Friedberg, Insel, & Spence)
Math 413/513 Chapter 6 (from Friedberg, Insel, & Spence) David Glickenstein December 7, 2015 1 Inner product spaces In this chapter, we will only consider the elds R and C. De nition 1 Let V be a vector
More informationOn divergence representations of the Gaussian and the mean curvature of surfaces and applications
Bull. Nov. Comp. Center, Math. Model. in Geoph., 17 (014), 35 45 c 014 NCC Publisher On divergence representations of the Gaussian and the mean curvature of surfaces and applications A.G. Megrabov Abstract.
More informationElectromagnetism HW 1 math review
Electromagnetism HW math review Problems -5 due Mon 7th Sep, 6- due Mon 4th Sep Exercise. The Levi-Civita symbol, ɛ ijk, also known as the completely antisymmetric rank-3 tensor, has the following properties:
More informationMathematical Relativity, Spring 2017/18 Instituto Superior Técnico
Mathematical Relativity, Spring 2017/18 Instituto Superior Técnico 1. Starting from R αβµν Z ν = 2 [α β] Z µ, deduce the components of the Riemann curvature tensor in terms of the Christoffel symbols.
More informationTime-Periodic Solutions of the Einstein s Field Equations II: Geometric Singularities
Science in China Series A: Mathematics 2009 Vol. 52 No. 11 1 16 www.scichina.com www.springerlink.com Time-Periodic Solutions of the Einstein s Field Equations II: Geometric Singularities KONG DeXing 1,
More informationE 2 = p 2 + m 2. [J i, J j ] = iɛ ijk J k
3.1. KLEIN GORDON April 17, 2015 Lecture XXXI Relativsitic Quantum Mechanics 3.1 Klein Gordon Before we get to the Dirac equation, let s consider the most straightforward derivation of a relativistically
More informationClass Meeting # 1: Introduction to PDEs
MATH 18.152 COURSE NOTES - CLASS MEETING # 1 18.152 Introduction to PDEs, Spring 2017 Professor: Jared Speck Class Meeting # 1: Introduction to PDEs 1. What is a PDE? We will be studying functions u =
More information16.20 HANDOUT #2 Fall, 2002 Review of General Elasticity
6.20 HANDOUT #2 Fall, 2002 Review of General Elasticity NOTATION REVIEW (e.g., for strain) Engineering Contracted Engineering Tensor Tensor ε x = ε = ε xx = ε ε y = ε 2 = ε yy = ε 22 ε z = ε 3 = ε zz =
More information8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS
8.821 F2008 Lecture 12: Boundary of AdS; Poincaré patch; wave equation in AdS Lecturer: McGreevy Scribe: Francesco D Eramo October 16, 2008 Today: 1. the boundary of AdS 2. Poincaré patch 3. motivate boundary
More informationInvariant Nonholonomic Riemannian Structures on Three-Dimensional Lie Groups
Invariant Nonholonomic Riemannian Structures on Three-Dimensional Lie Groups Dennis I. Barrett Geometry, Graphs and Control (GGC) Research Group Department of Mathematics (Pure and Applied) Rhodes University,
More informationM3/4A16 Assessed Coursework 1 Darryl Holm Due in class Thursday November 6, 2008 #1 Eikonal equation from Fermat s principle
D. D. Holm November 6, 2008 M3/416 Geom Mech Part 1 1 M3/416 ssessed Coursework 1 Darryl Holm Due in class Thursday November 6, 2008 #1 Eikonal equation from Fermat s principle #1a Prove that the 3D eikonal
More informationIntroduction of Partial Differential Equations and Boundary Value Problems
Introduction of Partial Differential Equations and Boundary Value Problems 2009 Outline Definition Classification Where PDEs come from? Well-posed problem, solutions Initial Conditions and Boundary Conditions
More informationOn universality of critical behaviour in Hamiltonian PDEs
Riemann - Hilbert Problems, Integrability and Asymptotics Trieste, September 23, 2005 On universality of critical behaviour in Hamiltonian PDEs Boris DUBROVIN SISSA (Trieste) 1 Main subject: Hamiltonian
More information