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A Scale-Covariant Quantum Space-Time
A scale-covariant quantum space-time Claudio Perini∗ Institute for Gravitation and the Cosmos, Physics Department, Penn State, University Park, PA 16802-6300, USA Gabriele Nunzio Tornetta† School of Mathematics and Statistics, University of Glasgow, 15 University Gardens, G12 8QW, Scotland A noncommutative space-time admitting dilation symmetry was briefly mentioned in the seminal work [1] of Doplicher, Fredenhagen and Roberts. In this paper we explicitly construct the model in details and carry out an in-depth analysis. The C∗-algebra that describes this quantum space-time is determined, and it is shown that it admits an action by - automorphisms of the dilation group, along with the expected Poincar´ecovariance. In order∗ to study the main physical properties of this scale-covariant model, a free scalar neutral field is introduced as a investigation tool. Our key results are then the loss of locality and the irreducibility, or triviality, of special field algebras associated with regions of the ordinary Minkowski space-time. It turns out, in the conclusions, that this analysis allows also to argue on viable ways of constructing a full conformally covariant model for quantum space-time. I. INTRODUCTION In this paper we study a non-commutative space-time of DFR-type, that can be obtained as the limiting scale-free case of the original DFR model [1]. The main mathematical interest to study this model is that it is Poincar´e and dilation covariant, thus it possesses almost all the symmetries given by the conformal group. The issue of implementing the remaining symmetry, which is the relativistic ray inversion, is discussed in the concluding section. -
On the Space of Generalized Fluxes for Loop Quantum Gravity
Home Search Collections Journals About Contact us My IOPscience On the space of generalized fluxes for loop quantum gravity This article has been downloaded from IOPscience. Please scroll down to see the full text article. 2013 Class. Quantum Grav. 30 055008 (http://iopscience.iop.org/0264-9381/30/5/055008) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 194.94.224.254 The article was downloaded on 07/03/2013 at 11:02 Please note that terms and conditions apply. IOP PUBLISHING CLASSICAL AND QUANTUM GRAVITY Class. Quantum Grav. 30 (2013) 055008 (24pp) doi:10.1088/0264-9381/30/5/055008 On the space of generalized fluxes for loop quantum gravity B Dittrich1,2, C Guedes1 and D Oriti1 1 Max Planck Institute for Gravitational Physics, Am Muhlenberg¨ 1, D-14476 Golm, Germany 2 Perimeter Institute for Theoretical Physics, 31 Caroline St N, Waterloo ON N2 L 2Y5, Canada E-mail: [email protected], [email protected] and [email protected] Received 5 September 2012, in final form 13 January 2013 Published 5 February 2013 Online at stacks.iop.org/CQG/30/055008 Abstract We show that the space of generalized fluxes—momentum space—for loop quantum gravity cannot be constructed by Fourier transforming the projective limit construction of the space of generalized connections—position space— due to the non-Abelianess of the gauge group SU(2). From the Abelianization of SU(2),U(1)3, we learn that the space of generalized fluxes turns out to be an inductive limit, and we determine the consistency conditions the fluxes should satisfy under coarse graining of the underlying graphs. -
Chapter 2 C -Algebras
Chapter 2 C∗-algebras This chapter is mainly based on the first chapters of the book [Mur90]. Material bor- rowed from other references will be specified. 2.1 Banach algebras Definition 2.1.1. A Banach algebra C is a complex vector space endowed with an associative multiplication and with a norm k · k which satisfy for any A; B; C 2 C and α 2 C (i) (αA)B = α(AB) = A(αB), (ii) A(B + C) = AB + AC and (A + B)C = AC + BC, (iii) kABk ≤ kAkkBk (submultiplicativity) (iv) C is complete with the norm k · k. One says that C is abelian or commutative if AB = BA for all A; B 2 C . One also says that C is unital if 1 2 C , i.e. if there exists an element 1 2 C with k1k = 1 such that 1B = B = B1 for all B 2 C . A subalgebra J of C is a vector subspace which is stable for the multiplication. If J is norm closed, it is a Banach algebra in itself. Examples 2.1.2. (i) C, Mn(C), B(H), K (H) are Banach algebras, where Mn(C) denotes the set of n × n-matrices over C. All except K (H) are unital, and K (H) is unital if H is finite dimensional. (ii) If Ω is a locally compact topological space, C0(Ω) and Cb(Ω) are abelian Banach algebras, where Cb(Ω) denotes the set of all bounded and continuous complex func- tions from Ω to C, and C0(Ω) denotes the subset of Cb(Ω) of functions f which vanish at infinity, i.e. -
Low-Dimensional Internal Categorial Structures in Weakly Mal'cev
Low-dimensional internal categorial structures in weakly Mal'cev sesquicategories N. Martins-Ferreira Polytechnic Institute of Leiria Thesis Presented for the Degree of DOCTOR OF PHILOSOPHY in the Department of Mathematics and Applied Mathematics UNIVERSITY OF CAPE TOWN June 3, 2008 ii Abstract In this work, the author introduces pseudocategory as a generalization for an internal category in dimension 2. First, a pseudocategory is de- ¯ned [Ch1]1 as a system, consisting of a precategory diagram together with special 2-cells in a 2-category, satisfying some coherence conditions: if the 2-category is of the form Cat(B), of internal categories, internal functors and internal natural transformations in some category B, then a pseudocategory in (internal to) Cat(B) simultaneously generalizes internal bicategory in B and internal double-category in B (it is a pseudo-double- category in B, using the terminology of M. Grandis and R. Par¶e);later, a pseudocategory is considered in the more general context of a sesquicate- gory [Ch2], with one of the main results of this thesis being the description of pseudocategories in (internal to) a weakly Mal'cev sesquicategory [Ch9]. The notions of weakly Mal'cev category and weakly Mal'cev sesquicat- egory are also new concepts that are introduced here. Weakly Mal'cev categories, generalize Mal'cev categories, and seem to be an appropriate setting for the study of internal categories and precategories: an internal category (here, as in a Mal'cev category) is completely determined by its underlying reflexive graph; but (here, unlike in a Mal'cev category) not every internal category is an internal groupoid [Ch3]. -
Dark Matter and Weak Signals of Quantum Spacetime
PHYSICAL REVIEW D 95, 065009 (2017) Dark matter and weak signals of quantum spacetime † ‡ Sergio Doplicher,1,* Klaus Fredenhagen,2, Gerardo Morsella,3, and Nicola Pinamonti4,§ 1Dipartimento di Matematica, Università di Roma “La Sapienza”, Piazzale Aldo Moro 5, I-00185 Roma, Italy 2II Institut für Theoretische Physik, Universität Hamburg, D-22761 Hamburg, Germany 3Dipartimento di Matematica, Università di Roma “Tor Vergata”, Via della Ricerca Scientifica, I-00133 Roma, Italy 4Dipartimento di Matematica, Università di Genova, Via Dodecaneso 35, I-16146 Genova, Italy, and INFN Sezione di Genova, Genova, Italy (Received 29 December 2016; published 13 March 2017) In physically motivated models of quantum spacetime, a Uð1Þ gauge theory turns into a Uð∞Þ gauge theory; hence, free classical electrodynamics is no longer free and neutral fields may have electromagnetic interactions. We discuss the last point for scalar fields, as a way to possibly describe dark matter; we have in mind the gravitational collapse of binary systems or future applications to self-gravitating Bose-Einstein condensates as possible sources of evidence of quantum gravitational phenomena. The effects considered so far, however, seem too faint to be detectable at present. DOI: 10.1103/PhysRevD.95.065009 I. INTRODUCTION but their superpositions would, in general, not be—they would lose energy in favor of mysterious massive modes One of the main difficulties of present-day physics is the (see also [6]). lack of observation of quantum aspects of gravity. Quantum A naive computation showed, by that mechanism, that a gravity has to be searched without a guide from nature; the monochromatic wave train passing through a partially observed universe must be explained as carrying traces of reflecting mirror should lose, in favor of those ghost quantum gravitational phenomena in the only “laboratory” modes, a fraction of its energy—a very small fraction, suitable to those effects, i.e., the universe itself a few unfortunately, of the order of one part in 10−130 [5]. -
The Principle of Locality. Effectiveness, Fate and Challenges
The Principle of Locality. Effectiveness, fate and challenges Sergio Doplicher Dipartimento di Matematica University of Rome “La Sapienza” 00185 Roma, Italy October 26, 2018 Abstract The Special Theory of Relativity and Quantum Mechanics merge in the key principle of Quantum Field Theory, the Principle of Locality. We review some examples of its “unreasonable effectiveness” in giving rise to most of the conceptual and structural frame of Quantum Field Theory, especially in absence of massless particles. This effectiveness shows up best in the formulation of Quantum Field Theory in terms of operator algebras of local observables; this formulation is successful in digging out the roots of Global Gauge Invariance, through the analysis of Superselection Structure and Statistics, in the structure of the local observable quantities alone, at least for purely massive theories; but so far it seems unfit to cope with the Principle of Local Gauge Invariance. This problem emerges also if one attempts to figure out the fate of the Principle of Locality in theories describing the gravitational forces between elementary particles as well. An approach based on the need to keep an operational meaning, in terms of localisation of events, of the notion of Spacetime, shows that, in the small, the latter must loose arXiv:0911.5136v1 [math-ph] 26 Nov 2009 any meaning as a classical pseudoRiemannian manifold, locally based on Minkowski space, but should acquire a quantum structure at the Planck scale. We review the Geometry of a basic model of Quantum Spacetime and some attempts to formulate interaction of quantum fields on Quan- tum Spacetime. The Principle of Locality is necessarily lost at the Planck scale, and it is a crucial open problem to unravel a replacement in such theories which is equally mathematically sharp, namely a Prin- ciple where the General Theory of Relativity and Quantum Mechanics merge, which reduces to the Principle of Locality at larger scales. -
Banach Algebras
Banach Algebras Yurii Khomskii Bachelor Thesis Department of Mathematics, Leiden University Supervisor: Dr. Marcel de Jeu April 18, 2005 i Contents Foreword iv 1. Algebraic Concepts 1 1.1. Preliminaries . 1 1.2. Regular Ideals . 3 1.3. Adjoining an Identity . 4 1.4. Quasi-inverses . 8 2. Banach Algebras 10 2.1. Preliminaries of Normed and Banach Algebras . 10 2.2. Inversion and Quasi-inversion in Banach Algebras . 14 3. Spectra 18 3.1. Preliminaries . 18 3.2. Polynomial Spectral Mapping Theorem and the Spectral Radius Formula . 22 4. Gelfand Representation Theory 25 4.1. Multiplicative Linear Functionals and the Maximal Ideal Space . 25 4.2. The Gelfand Topology . 30 4.3. The Gelfand Representation . 31 4.4. The Radical and Semi-simplicity . 33 4.5. Generators of Banach algebras . 34 5. Examples of Gelfand Representations 36 5.1. C (X ) for X compact and Hausdorff . 36 5.2. C 0(X ) for X locally compact and Hausdorff. 41 5.3. Stone-Cecˇ h compactification . 42 5.4. A(D) . 44 5.5. AC (Γ) . 46 5.6. H 1 . 47 ii iii Foreword The study of Banach algebras began in the twentieth century and originated from the observation that some Banach spaces show interesting properties when they can be supplied with an extra multiplication operation. A standard exam- ple was the space of bounded linear operators on a Banach space, but another important one was function spaces (of continuous, bounded, vanishing at infin- ity etc. functions as well as functions with absolutely convergent Fourier series). Nowadays Banach algebras is a wide discipline with a variety of specializations and applications. -
Mathematical Tripos Part III Lecture Courses in 2013-2014
Mathematical Tripos Part III Lecture Courses in 2013-2014 Department of Pure Mathematics & Mathematical Statistics Department of Applied Mathematics & Theoretical Physics Notes and Disclaimers. • Students may take any combination of lectures that is allowed by the timetable. The examination timetable corresponds to the lecture timetable and it is therefore not possible to take two courses for examination that are lectured in the same timetable slot. There is no requirement that students study only courses offered by one Department. • The code in parentheses after each course name indicates the term of the course (M: Michaelmas; L: Lent; E: Easter), and the number of lectures in the course. Unless indicated otherwise, a 16 lecture course is equivalent to 2 credit units, while a 24 lecture course is equivalent to 3 credit units. Please note that certain courses are non-examinable, and are indicated as such after the title. Some of these courses may be the basis for Part III essays. • At the start of some sections there is a paragraph indicating the desirable previous knowledge for courses in that section. On one hand, such paragraphs are not exhaustive, whilst on the other, not all courses require all the pre-requisite material indicated. However you are strongly recommended to read up on the material with which you are unfamiliar if you intend to take a significant number of courses from a particular section. • The courses described in this document apply only for the academic year 2013-14. Details for subsequent years are often broadly similar, but not necessarily identical. The courses evolve from year to year. -
Spectral Theory
SPECTRAL THEORY EVAN JENKINS Abstract. These are notes from two lectures given in MATH 27200, Basic Functional Analysis, at the University of Chicago in March 2010. The proof of the spectral theorem for compact operators comes from [Zim90, Chapter 3]. 1. The Spectral Theorem for Compact Operators The idea of the proof of the spectral theorem for compact self-adjoint operators on a Hilbert space is very similar to the finite-dimensional case. Namely, we first show that an eigenvector exists, and then we show that there is an orthonormal basis of eigenvectors by an inductive argument (in the form of an application of Zorn's lemma). We first recall a few facts about self-adjoint operators. Proposition 1.1. Let V be a Hilbert space, and T : V ! V a bounded, self-adjoint operator. (1) If W ⊂ V is a T -invariant subspace, then W ? is T -invariant. (2) For all v 2 V , hT v; vi 2 R. (3) Let Vλ = fv 2 V j T v = λvg. Then Vλ ? Vµ whenever λ 6= µ. We will need one further technical fact that characterizes the norm of a self-adjoint operator. Lemma 1.2. Let V be a Hilbert space, and T : V ! V a bounded, self-adjoint operator. Then kT k = supfjhT v; vij j kvk = 1g. Proof. Let α = supfjhT v; vij j kvk = 1g. Evidently, α ≤ kT k. We need to show the other direction. Given v 2 V with T v 6= 0, setting w0 = T v=kT vk gives jhT v; w0ij = kT vk. -
Adiabatic Limits and Renormalization in Quantum Spacetime
DOTTORATO DI RICERCA IN MATEMATICA XXXII CICLO DEL CORSO DI DOTTORATO Adiabatic limits and renormalization in quantum spacetime Aleksei Bykov A.A. 2019/2020 Docente Guida/Tutor: Prof. D. Guido Relatore: Prof. G. Morsella Coordinatore: Prof. A. Braides Contents 1 Introduction 4 2 Doplicher-Fredenhagen-Roberts Quantum Spacetime 11 2.1 Construction and basic facts . 11 2.2 Quantum fields on the DFR QST and the role of Qµν . 12 2.2.1 More general quantum fields in DFR QST . 13 2.3 Optimally localised states and the quantum diagonal map . 17 3 Perturbation theory for QFT and its non-local generalization 21 3.1 Hamiltonian perturbation theory . 22 3.1.1 Ordinary QFT . 22 3.1.2 Non-local case: fixing HI ............................. 26 3.1.3 Hamiltonian approach: fixing Hint ........................ 35 3.2 Lagrangian perturbation theories . 38 3.3 Yang-Feldman quantizaion . 41 3.4 LSZ reduction . 41 4 Feynman rules for non-local Hamiltonian Perturbation theory 45 5 Lagrangian reformulation of the Hamiltonian Feynman rules 52 6 Corrected propagator 57 7 Adiabatic limit 61 7.1 Weak adiabatic limit and the LSZ reduction . 61 7.1.1 Existence of the weak adiabatic limit . 61 7.1.2 Feynman rules from LSZ reduction . 64 7.2 Strong adiabatic limit . 65 8 Renormalization 68 8.1 Formal renormalization . 68 8.2 The physical renormalization . 71 8.2.1 Dispersion relation renormalisation . 72 8.2.2 Field strength renormalization . 72 8.3 Conluding remarks on renormalisation . 73 9 Conclusions 75 9.1 Summary of the main results . 75 9.2 Outline of further directions . -
The Periodic Table of N-Categories for Low Dimensions I: Degenerate Categories and Degenerate Bicategories Draft
The periodic table of n-categories for low dimensions I: degenerate categories and degenerate bicategories draft Eugenia Cheng and Nick Gurski Department of Mathematics University of Chicago E-mail: [email protected], [email protected] July 2005 Abstract We examine the periodic table of weak n-categories for the low-dimensional cases. It is widely understood that degenerate categories give rise to monoids, doubly degenerate bicategories to commutative monoids, and degenerate bicategories to monoidal categories; however, to understand this correspondence fully we examine the totalities of such structures to- gether with maps between them and higher maps between those. Cate- gories naturally form a 2-category Cat so we take the full sub-2-category of this whose 0-cells are the degenerate categories. Monoids naturally form a category, but we regard this as a discrete 2-category to make the comparison. We show that this construction does not yield a biequiva- lence; to get an equivalence we ignore the natural transformations and consider only the category of degenerate categories. A similar situation occurs for degenerate bicategories. The tricategory of such does not yield an equivalence with monoidal categories; we must consider only the cate- gories of such structures. For doubly degenerate bicategories the tricate- gory of such is not naturally triequivalent to the category of commutative monoids (regarded as a tricategory). However in this case considering just the categories does not give an equivalence either; to get an equivalence we consider the bicategory of doubly degenerate bicategories. We conclude with a hypothesis about how the above cases might generalise for n-fold degenerate n-categories. -
MAT 449 : Representation Theory
MAT 449 : Representation theory Sophie Morel December 17, 2018 Contents I Representations of topological groups5 I.1 Topological groups . .5 I.2 Haar measures . .9 I.3 Representations . 17 I.3.1 Continuous representations . 17 I.3.2 Unitary representations . 20 I.3.3 Cyclic representations . 24 I.3.4 Schur’s lemma . 25 I.3.5 Finite-dimensional representations . 27 I.4 The convolution product and the group algebra . 28 I.4.1 Convolution on L1(G) and the group algebra of G ............ 28 I.4.2 Representations of G vs representations of L1(G) ............. 33 I.4.3 Convolution on other Lp spaces . 39 II Some Gelfand theory 43 II.1 Banach algebras . 43 II.1.1 Spectrum of an element . 43 II.1.2 The Gelfand-Mazur theorem . 47 II.2 Spectrum of a Banach algebra . 48 II.3 C∗-algebras and the Gelfand-Naimark theorem . 52 II.4 The spectral theorem . 55 III The Gelfand-Raikov theorem 59 III.1 L1(G) ....................................... 59 III.2 Functions of positive type . 59 III.3 Functions of positive type and irreducible representations . 65 III.4 The convex set P1 ................................. 68 III.5 The Gelfand-Raikov theorem . 73 IV The Peter-Weyl theorem 75 IV.1 Compact operators . 75 IV.2 Semisimplicity of unitary representations of compact groups . 77 IV.3 Matrix coefficients . 80 IV.4 The Peter-Weyl theorem . 86 IV.5 Characters . 87 3 Contents IV.6 The Fourier transform . 90 IV.7 Characters and Fourier transforms . 93 V Gelfand pairs 97 V.1 Invariant and bi-invariant functions .