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Functional Analysis Lecture Notes Chapter 2. Operators on Hilbert Spaces
FUNCTIONAL ANALYSIS LECTURE NOTES CHAPTER 2. OPERATORS ON HILBERT SPACES CHRISTOPHER HEIL 1. Elementary Properties and Examples First recall the basic definitions regarding operators. Definition 1.1 (Continuous and Bounded Operators). Let X, Y be normed linear spaces, and let L: X Y be a linear operator. ! (a) L is continuous at a point f X if f f in X implies Lf Lf in Y . 2 n ! n ! (b) L is continuous if it is continuous at every point, i.e., if fn f in X implies Lfn Lf in Y for every f. ! ! (c) L is bounded if there exists a finite K 0 such that ≥ f X; Lf K f : 8 2 k k ≤ k k Note that Lf is the norm of Lf in Y , while f is the norm of f in X. k k k k (d) The operator norm of L is L = sup Lf : k k kfk=1 k k (e) We let (X; Y ) denote the set of all bounded linear operators mapping X into Y , i.e., B (X; Y ) = L: X Y : L is bounded and linear : B f ! g If X = Y = X then we write (X) = (X; X). B B (f) If Y = F then we say that L is a functional. The set of all bounded linear functionals on X is the dual space of X, and is denoted X0 = (X; F) = L: X F : L is bounded and linear : B f ! g We saw in Chapter 1 that, for a linear operator, boundedness and continuity are equivalent. -
Bounds of Eigenvalues on Riemannian Manifolds, Trends In
Trends in °c Higher Education Press Partial Di®erential Equations and International Press ALM 10, pp. 241{264 Beijing-Boston Bounds of Eigenvalues on Riemannian Manifolds Jun Ling¤ Zhiqin Luy Abstract In this paper, we ¯rst give a short review of the eigenvalue estimates of Laplace operator and SchrÄodingeroperators. Then we discuss the evolution of eigenvalues along the Ricci flow, and two new bounds of the ¯rst eigenvalue using gradient estimates. 2000 Mathematics Subject Classi¯cation: 58J50, 35P15, 53C21. Keywords and Phrases: Eigenvalue, lower bounds, upper bounds, Riemannian manifolds. 1 Introduction In this paper, we discuss the eigenvalue estimates of Laplace operator and SchrÄodin- ger operators. Let (M; g) be an n-dimensional compact connected Riemannian manifold with or without boundary. Let ¢ be the Laplacian of the metric g = i n (gij)n£n. In local coordinates fx gi=1, µ ¶ 1 Xn @ p @ ¢ = p det(g) gij ; @xi @xj det(g) i;j=1 ij where the matrix (g ) is the inverse matrix of g = (gij). We consider the following three eigenvalue problems on the manifold (M; g). ¤Department of Mathematics, Utah Valley University, Orem, UT 84058, USA. Email: [email protected]. Research partially supported by the NSF under the program `The Geomet- ric Evolution Equations and Related Topics' at the MSRI at Berkeley and by the UVU School of Science and Health. yDepartment of Mathematics, University of California, Irvine, CA 92697, USA. Email: [email protected]. Research partially supported by NSF grant DMS 0347033. 242 J. Ling and Z. Lu Closed eigenvalue problem for the Laplacian. @M = ;. Find all real numbers ¸ for which there are nontrivial solutions u 2 C2(M) to the equations ¡¢u = ¸u: (1.1) Dirichlet eigenvalue problem for the Laplacian. -
Heat Kernels and Green's Functions on Limit Spaces
HEAT KERNELS AND GREEN'S FUNCTIONS ON LIMIT SPACES YU DING Abstract. In this paper, we study the behavior of the Laplacian on a sequence of n manifolds fMi g with a lower bound in Ricci curvature that converges to a metric- measure space M1. We prove that the heat kernels and Green's functions on n Mi will converge to some integral kernels on M1 which can be interpreted, in different cases, as the heat kernel and Green's function on M1. We also study the Laplacian on noncollapsed metric cones; these provide a unified treatment of the asymptotic behavior of heat kernels and Green's functions on noncompact manifolds with nonnegative Ricci curvature and Euclidean volume growth. In particular, we get a unified proof of the asymptotic formulae of Colding-Minicozzi, Li and Li-Tam- Wang. Introduction Assume M n is an n dimensional Riemannian manifold with a lower bound in Ricci curvature, (0.1) RicM n ≥ −(n − 1)Λ; where Λ ≥ 0. By the Bishop-Gromov inequality, we have a uniform volume doubling condition, κ (0.2) Vol(B2R(p)) ≤ 2 Vol(BR(p)); here we can take κ = n if Λ = 0; if Λ > 0, we require that R is bounded from above, say, R < D for some D > 0. Moreover, there is a uniform Poincare inequality Z Z 1 1 2 1 (0.3) jf − fp;Rj ≤ τR( jdfj ) 2 ; Vol(BR(p)) BR(p) Vol(BR(p)) BR(p) where fp;R is the average of f on BR(p); see [Bu], [Ch3], [HaKo] and the references therein. -
Quantum Mechanics, Schrodinger Operators and Spectral Theory
Quantum mechanics, SchrÄodingeroperators and spectral theory. Spectral theory of SchrÄodinger operators has been my original ¯eld of expertise. It is a wonderful mix of functional analy- sis, PDE and Fourier analysis. In quantum mechanics, every physical observable is described by a self-adjoint operator - an in¯nite dimensional symmetric matrix. For example, ¡¢ is a self-adjoint operator in L2(Rd) when de¯ned on an appropriate domain (Sobolev space H2). In quantum mechanics it corresponds to a free particle - just traveling in space. What does it mean, exactly? Well, in quantum mechanics, position of a particle is described by a wave 2 d function, Á(x; t) 2 L (R ): The physical meaningR of the wave function is that the probability 2 to ¯nd it in a region at time t is equal to jÁ(x; t)j dx: You can't know for sure where the particle is for sure. If initially the wave function is given by Á(x; 0) = Á0(x); the SchrÄodinger ¡i¢t equation says that its evolution is given by Á(x; t) = e Á0: But how to compute what is e¡i¢t? This is where Fourier transform comes in handy. Di®erentiation becomes multiplication on the Fourier transform side, and so Z ¡i¢t ikx¡ijkj2t ^ e Á0(x) = e Á0(k) dk; Rd R ^ ¡ikx where Á0(k) = Rd e Á0(x) dx is the Fourier transform of Á0: I omitted some ¼'s since they do not change the picture. Stationary phase methods lead to very precise estimates on free SchrÄodingerevolution. -
Operator Algebras: an Informal Overview 3
OPERATOR ALGEBRAS: AN INFORMAL OVERVIEW FERNANDO LLEDO´ Contents 1. Introduction 1 2. Operator algebras 2 2.1. What are operator algebras? 2 2.2. Differences and analogies between C*- and von Neumann algebras 3 2.3. Relevance of operator algebras 5 3. Different ways to think about operator algebras 6 3.1. Operator algebras as non-commutative spaces 6 3.2. Operator algebras as a natural universe for spectral theory 6 3.3. Von Neumann algebras as symmetry algebras 7 4. Some classical results 8 4.1. Operator algebras in functional analysis 8 4.2. Operator algebras in harmonic analysis 10 4.3. Operator algebras in quantum physics 11 References 13 Abstract. In this article we give a short and informal overview of some aspects of the theory of C*- and von Neumann algebras. We also mention some classical results and applications of these families of operator algebras. 1. Introduction arXiv:0901.0232v1 [math.OA] 2 Jan 2009 Any introduction to the theory of operator algebras, a subject that has deep interrelations with many mathematical and physical disciplines, will miss out important elements of the theory, and this introduction is no ex- ception. The purpose of this article is to give a brief and informal overview on C*- and von Neumann algebras which are the main actors of this summer school. We will also mention some of the classical results in the theory of operator algebras that have been crucial for the development of several areas in mathematics and mathematical physics. Being an overview we can not provide details. Precise definitions, statements and examples can be found in [1] and references cited therein. -
STRUCTURE of the LAPLACIAN on BOUNDED DOMAINS Contents 1. Introduction 1 2. Rellich's Compactness Lemma 4 3. Spectral Theory O
STRUCTURE OF THE LAPLACIAN ON BOUNDED DOMAINS TSOGTGEREL GANTUMUR Contents 1. Introduction1 2. Rellich’s compactness lemma4 3. Spectral theory of compact self-adjoint operators9 4. Application to the Laplace eigenproblems 12 5. Courant’s minimax principle 16 6. Weyl’s asymptotic law 19 7. Problems and exercises 21 1. Introduction In this chapter, we will be concerned with the eigenvalue problem − ∆u = λu, (1) n in a bounded open set Ω ⊂ R , with either the Dirichlet u = 0 or the Neumann @νu = 0 condition on the boundary @Ω. The unknown in the problem is the pair (u; λ) where u is a function and λ is a number. If (u; λ) is a solution then u is called an eigenfunction, and λ is called the eigenvalue associated to u. Let us note the following. • Since the right hand side involves λu, the problem is not linear. • If (u; λ) is a solution then so is (αu; λ) for any number α. • We exclude the trivial solution u = 0 from all considerations. We have studied the problem −∆u+tu = f with the Dirichlet or Neumann boundary conditions, 2 where t 2 R and f 2 L (Ω) are given. Since (1) is equivalent to −∆u + tu = 0 with t = −λ, we 1 1 can give the following weak formulation for (1). Let V be either H0 (Ω) or H (Ω), depending on the boundary condition we wish to impose. Then the problem is to find u 2 V and λ 2 R satisfying Z Z ru · rv = λ uv for all v 2 V: (2) Ω Ω We know that a unique weak solution u 2 V to −∆u + tu = f exists if t > t0, where t0 = 0 for the Neumann case, and t0 < 0 for the Dirichlet case. -
Functional Analysis (WS 19/20), Problem Set 8 (Spectrum And
Functional Analysis (WS 19/20), Problem Set 8 (spectrum and adjoints on Hilbert spaces)1 In what follows, let H be a complex Hilbert space. Let T : H ! H be a bounded linear operator. We write T ∗ : H ! H for adjoint of T dened with hT x; yi = hx; T ∗yi: This operator exists and is uniquely determined by Riesz Representation Theorem. Spectrum of T is the set σ(T ) = fλ 2 C : T − λI does not have a bounded inverseg. Resolvent of T is the set ρ(T ) = C n σ(T ). Basic facts on adjoint operators R1. | Adjoint T ∗ exists and is uniquely determined. R2. | Adjoint T ∗ is a bounded linear operator and kT ∗k = kT k. Moreover, kT ∗T k = kT k2. R3. | Taking adjoints is an involution: (T ∗)∗ = T . R4. Adjoints commute with the sum: ∗ ∗ ∗. | (T1 + T2) = T1 + T2 ∗ ∗ R5. | For λ 2 C we have (λT ) = λ T . R6. | Let T be a bounded invertible operator. Then, (T ∗)−1 = (T −1)∗. R7. Let be bounded operators. Then, ∗ ∗ ∗. | T1;T2 (T1 T2) = T2 T1 R8. | We have relationship between kernel and image of T and T ∗: ker T ∗ = (im T )?; (ker T ∗)? = im T It will be helpful to prove that if M ⊂ H is a linear subspace, then M = M ??. Btw, this covers all previous results like if N is a nite dimensional linear subspace then N = N ?? (because N is closed). Computation of adjoints n n ∗ M1. ,Let A : R ! R be a complex matrix. Find A . 2 M2. | ,Let H = l (Z). For x = (:::; x−2; x−1; x0; x1; x2; :::) 2 H we dene the right shift operator −1 ∗ with (Rx)k = xk−1: Find kRk, R and R . -
Scattering Theory
Scattering Theory Sean Harris October 2016 A thesis submitted for the degree of Bachelor of Philosophy (Honours) of the Australian National University Declaration The work in this thesis is my own except where otherwise stated. The first four chapters are largely expository, covering background material. The final two chapters contain mostly new theorems (to the best of my knowledge) proven by myself, with some help by others such as Professor Andrew Hassell. Sean Harris Acknowledgements Most of all I would like to thank my supervisor Professor Andrew Hassell, for developing my interest in this topic, always finding time to meet with me to discuss issues, and being generally great. I am also incredibly grateful to Dr Melissa Tacy for helping me draft this thesis while Andrew was absent. Thanks also goes to the many lecturers I have met leading up to this moment, for nourishing my interest in mathematics. My fellow Dungeon-dwelling honours students have also been incredibly helpful throughout the year. Special mention to Hugh McCarthy, for always being available to chat about any problems I was having (both mathematical and otherwise). A few more people to mention: my tutorial students, for giving me some reprieve from study; the staff at the ANU Food Co-op, for the great lunches (I wish I had discovered them earlier); and the many green envelopes and the single red envelope, for keeping me going. I guess I should thank my parents too. v Abstract Scattering theory studies the comparison between evolution obeying \free dynamics" and evolution obeying some \perturbed dynamics". The asymptotic nature of free and perturbed evolution are compared to determine properties of the perturbation. -
Quantum Dynamics
Quantum Dynamics William G. Faris August 12, 1992 Contents I Hilbert Space 5 1 Introduction 7 1.1 Quantum mechanics . 7 1.2 The quantum scale . 8 1.2.1 Planck's constant . 8 1.2.2 Diffusion . 9 1.2.3 Speed . 9 1.2.4 Length . 10 1.2.5 Energy . 10 1.2.6 Compressibility . 10 1.2.7 Frequency . 11 1.2.8 Other length scales . 11 1.3 The Schr¨odingerequation . 11 1.3.1 The equation . 11 1.3.2 Density and current . 13 1.3.3 Osmotic and current velocity . 14 1.3.4 Momentum . 15 1.3.5 Energy . 15 1.4 The uncertainty principle . 17 1.5 Quantum stability . 18 2 Hilbert Space 21 2.1 Definition . 21 2.2 Self-duality . 24 2.3 Projections . 26 2.4 Operators . 27 2.5 Bounded operators . 28 1 2 CONTENTS 3 Function Spaces 31 3.1 Integration . 31 3.2 Function spaces . 34 3.3 Convergence . 36 3.4 Integral operators . 37 4 Bases 41 4.1 Discrete bases . 41 4.2 Continuous bases . 42 5 Spectral Representations 49 5.1 Multiplication operators . 49 5.2 Spectral representations . 50 5.3 Translation . 52 5.4 Approximate delta functions . 53 5.5 The Fourier transform . 54 5.6 Free motion . 57 5.6.1 Diffusion . 57 5.6.2 Oscillation . 58 6 The Harmonic Oscillator 61 6.1 The classical harmonic oscillator . 61 6.2 The one dimensional quantum harmonic oscillator . 62 6.3 The Fourier transform . 65 6.4 Density theorems . 65 6.5 The isotropic quantum harmonic oscillator . -
Notes on Von Neumann Algebras
Notes on von Neumann algebras Jesse Peterson April 5, 2013 2 Chapter 1 Spectral theory If A is a complex unital algebra then we denote by G(A) the set of elements which have a two sided inverse. If x 2 A, the spectrum of x is σA(x) = fλ 2 C j x − λ 62 G(A)g: The complement of the spectrum is called the resolvent and denoted ρA(x). Proposition 1.0.1. Let A be a unital algebra over C, and consider x; y 2 A. Then σA(xy) [ f0g = σA(yx) [ f0g. Proof. If 1 − xy 2 G(A) then we have (1 − yx)(1 + y(1 − xy)−1x) = 1 − yx + y(1 − xy)−1x − yxy(1 − xy)−1x = 1 − yx + y(1 − xy)(1 − xy)−1x = 1: Similarly, we have (1 + y(1 − xy)−1x)(1 − yx) = 1; and hence 1 − yx 2 G(A). Knowing the formula for the inverse beforehand of course made the proof of the previous proposition quite a bit easier. But this formula is quite natural to consider. Indeed, if we just consider formal power series then we have 1 1 X X (1 − yx)−1 = (yx)k = 1 + y( (xy)k)x = 1 + y(1 − xy)−1x: k=0 k=0 1.1 Banach and C∗-algebras A Banach algebra is a Banach space A, which is also an algebra such that kxyk ≤ kxkkyk: 3 4 CHAPTER 1. SPECTRAL THEORY A Banach algebra A is involutive if it possesses an anti-linear involution ∗, such that kx∗k = kxk, for all x 2 A. -
Notes on Von Neumann Algebras
Von Neumann Algebras. Vaughan F.R. Jones 1 October 1, 2009 1Supported in part by NSF Grant DMS93–22675, the Marsden fund UOA520, and the Swiss National Science Foundation. 2 Chapter 1 Introduction. The purpose of these notes is to provide a rapid introduction to von Neumann algebras which gets to the examples and active topics with a minimum of technical baggage. In this sense it is opposite in spirit from the treatises of Dixmier [], Takesaki[], Pedersen[], Kadison-Ringrose[], Stratila-Zsido[]. The philosophy is to lavish attention on a few key results and examples, and we prefer to make simplifying assumptions rather than go for the most general case. Thus we do not hesitate to give several proofs of a single result, or repeat an argument with different hypotheses. The notes are built around semester- long courses given at UC Berkeley though they contain more material than could be taught in a single semester. The notes are informal and the exercises are an integral part of the ex- position. These exercises are vital and mostly intended to be easy. 3 4 Chapter 2 Background and Prerequisites 2.1 Hilbert Space A Hilbert Space is a complex vector space H with inner product h; i : HxH! C which is linear in the first variable, satisfies hξ; ηi = hη; ξi, is positive definite, i.e. hξ; ξi > 0 for ξ 6= 0, and is complete for the norm defined by test jjξjj = phξ; ξi. Exercise 2.1.1. Prove the parallelogram identity : jjξ − ηjj2 + jjξ + ηjj2 = 2(jjξjj2 + jjηjj2) and the Cauchy-Schwartz inequality: jhξ; ηij ≤ jjξjj jjηjj: Theorem 2.1.2. -
Spectrum (Functional Analysis) - Wikipedia, the Free Encyclopedia
Spectrum (functional analysis) - Wikipedia, the free encyclopedia http://en.wikipedia.org/wiki/Spectrum_(functional_analysis) Spectrum (functional analysis) From Wikipedia, the free encyclopedia In functional analysis, the concept of the spectrum of a bounded operator is a generalisation of the concept of eigenvalues for matrices. Specifically, a complex number λ is said to be in the spectrum of a bounded linear operator T if λI − T is not invertible, where I is the identity operator. The study of spectra and related properties is known as spectral theory, which has numerous applications, most notably the mathematical formulation of quantum mechanics. The spectrum of an operator on a finite-dimensional vector space is precisely the set of eigenvalues. However an operator on an infinite-dimensional space may have additional elements in its spectrum, and may have no eigenvalues. For example, consider the right shift operator R on the Hilbert space ℓ2, This has no eigenvalues, since if Rx=λx then by expanding this expression we see that x1=0, x2=0, etc. On the other hand 0 is in the spectrum because the operator R − 0 (i.e. R itself) is not invertible: it is not surjective since any vector with non-zero first component is not in its range. In fact every bounded linear operator on a complex Banach space must have a non-empty spectrum. The notion of spectrum extends to densely-defined unbounded operators. In this case a complex number λ is said to be in the spectrum of such an operator T:D→X (where D is dense in X) if there is no bounded inverse (λI − T)−1:X→D.