Unit 4 String Theory and Extra Dimensions Introduction
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Confinement and Exotic Meson Spectroscopy at 12Gev JLAB
174 Brazilian Journal of Physics, vol. 33, no. 2, June, 2003 Confinement and Exotic Meson Spectroscopy at 12GeV JLAB Adam Szczepaniak Physics Department, Indiana University, Bloomington, IN 47405, USA Received on 30 October, 2002 Phenomenology of gluonic excitations and possibilities for searches of exotic mesons at JLab are discussed. I Introduction O(104) number. For technical reasons dynamical evolu- tion is studied by replacing the Minkowski by the Euclidean Quantum chromodynamics (QCD) represents part of the metric thereby converting to a statistical systems and using Standard Model which describes the strong interactions. Monte Carlo methods to evaluate the partition function. The fundamental degrees of freedom are quarks – the mat- In parallel many analytical many-body techniques have ter fields, and gluons – the mediators of the strong force. been employed to identify effective degrees of freedom and Quarks and gluons are permanently confined into hadrons, numerous approximation schemes have been advanced to e.g. protons, neutrons and pions, to within distance scales describe the soft structure and interactions of hadrons, e.g. of the order of 1fm = 10¡15m. Hadrons are bound by the constituent quark model, bag and topological soliton residual strong forces to form atomic nuclei. Thus QCD models, QCD sum rules, chiral lagrangians, etc. determines not only the quark-gluon dynamics at the sub- In this talk I will focus on the physics of soft gluonic ex- subatomic scale but also the interactions between nuclei at citations and their role in quark confinement. Gluons carry the subatomic scale and even the nuclear dynamics at a the strong force, and since on a hadronic scale the light u and macroscopic level, e.g. -
Not Even Wrong, Ten Years Later: a View from Mathematics on Prospects for Fundamental Physics Without Experiment
Not Even Wrong, ten years later: a view from mathematics on prospects for fundamental physics without experiment Peter Woit Columbia University Rutgers Physics Colloquium, February 3, 2016 Peter Woit (Columbia University) Not Even Wrong, ten years later: a view from mathematicsFebruary on prospects 3, 2016 for fundamental 1 / 32 physics without experiment Outline Some advertisements and some provocations: Advertisements: an old book, an ongoing blog, and a forthcoming book. Review what has happened to the idea of string theory unification. Raise the issue of what happens absent new experimental guidance. Can the example of mathematics help? Evidence for deep connections between math and physics: quantum mechanics and representation theory Speculation about relevance of ideas from representation theory to better understanding the Standard Model. Peter Woit (Columbia University) Not Even Wrong, ten years later: a view from mathematicsFebruary on prospects 3, 2016 for fundamental 2 / 32 physics without experiment An advertisment for three projects Not Even Wrong: the book Written largely in 2001-2 2003: under review at Cambridge University Press Fall 2004: accepted for publication by British publisher (with help from Roger Penrose) Mid-2006: published around same time as Lee Smolin's The Trouble with Physics. The \String Wars" kick off. Peter Woit (Columbia University) Not Even Wrong, ten years later: a view from mathematicsFebruary on prospects 3, 2016 for fundamental 3 / 32 physics without experiment An advertisment for three projects Not Even Wrong: the blog Started March 2004 In 2006, one of the battlefields of the string wars. Currently 1512 postings 41,335 comments Around 20,000 page-views/day (mostly robots...) http://www.math.columbia.edu/~woit/blog Peter Woit (Columbia University) Not Even Wrong, ten years later: a view from mathematicsFebruary on prospects 3, 2016 for fundamental 4 / 32 physics without experiment An advertisment for three projects An advertisement for the competition Finally in 2015, a book with the counter-argument I was expecting. -
Kaluza-Klein Gravity, Concentrating on the General Rel- Ativity, Rather Than Particle Physics Side of the Subject
Kaluza-Klein Gravity J. M. Overduin Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, British Columbia, Canada, V8W 3P6 and P. S. Wesson Department of Physics, University of Waterloo, Ontario, Canada N2L 3G1 and Gravity Probe-B, Hansen Physics Laboratories, Stanford University, Stanford, California, U.S.A. 94305 Abstract We review higher-dimensional unified theories from the general relativity, rather than the particle physics side. Three distinct approaches to the subject are identi- fied and contrasted: compactified, projective and noncompactified. We discuss the cosmological and astrophysical implications of extra dimensions, and conclude that none of the three approaches can be ruled out on observational grounds at the present time. arXiv:gr-qc/9805018v1 7 May 1998 Preprint submitted to Elsevier Preprint 3 February 2008 1 Introduction Kaluza’s [1] achievement was to show that five-dimensional general relativity contains both Einstein’s four-dimensional theory of gravity and Maxwell’s the- ory of electromagnetism. He however imposed a somewhat artificial restriction (the cylinder condition) on the coordinates, essentially barring the fifth one a priori from making a direct appearance in the laws of physics. Klein’s [2] con- tribution was to make this restriction less artificial by suggesting a plausible physical basis for it in compactification of the fifth dimension. This idea was enthusiastically received by unified-field theorists, and when the time came to include the strong and weak forces by extending Kaluza’s mechanism to higher dimensions, it was assumed that these too would be compact. This line of thinking has led through eleven-dimensional supergravity theories in the 1980s to the current favorite contenders for a possible “theory of everything,” ten-dimensional superstrings. -
ABSTRACT Investigation Into Compactified Dimensions: Casimir
ABSTRACT Investigation into Compactified Dimensions: Casimir Energies and Phenomenological Aspects Richard K. Obousy, Ph.D. Chairperson: Gerald B. Cleaver, Ph.D. The primary focus of this dissertation is the study of the Casimir effect and the possibility that this phenomenon may serve as a mechanism to mediate higher dimensional stability, and also as a possible mechanism for creating a small but non- zero vacuum energy density. In chapter one we review the nature of the quantum vacuum and discuss the different contributions to the vacuum energy density arising from different sectors of the standard model. Next, in chapter two, we discuss cosmology and the introduction of the cosmological constant into Einstein's field equations. In chapter three we explore the Casimir effect and study a number of mathematical techniques used to obtain a finite physical result for the Casimir energy. We also review the experiments that have verified the Casimir force. In chapter four we discuss the introduction of extra dimensions into physics. We begin by reviewing Kaluza Klein theory, and then discuss three popular higher dimensional models: bosonic string theory, large extra dimensions and warped extra dimensions. Chapter five is devoted to an original derivation of the Casimir energy we derived for the scenario of a higher dimensional vector field coupled to a scalar field in the fifth dimension. In chapter six we explore a range of vacuum scenarios and discuss research we have performed regarding moduli stability. Chapter seven explores a novel approach to spacecraft propulsion we have proposed based on the idea of manipulating the extra dimensions of string/M theory. -
Arxiv:0711.0760V3 [Hep-Th]
DBI N-flation John Ward1 Department of Physics and Astronomy, University of Victoria, Victoria BC, V8P 1A1, Canada Abstract We investigate DBI inflation using N multiple branes and show how the configuration is equivalent to a single wrapped D5-brane with flux. We then show how 1/N corrections can be implemented, and we examine the sound speed and levels of non-Gaussianities in two distinct cases. For models with constant warping we find that the non-Gaussian amplitude is bounded from above (as a function of γ). For AdS backgrounds we find that the signature is generally large and positive, although is no longer globally defined over the full phase space. We then investigate an inflationary mechanism using a representation cascade, whereby the transition from a reducible representation to the irrep drives inflation. arXiv:0711.0760v3 [hep-th] 26 Nov 2007 [email protected] 1 Introduction In the absence of any direct test of string theory, cosmology remains the best laboratory with which to test string theoretic models [1]. Over the past few years we have witnessed cosmology become a precision science, with COBE, WMAP and SDSS [2] providing crucial support for the flatness of the universe, the existence of dark energy and for a period of cosmic inflation. Whilst the dark energy puzzle remains an outstanding problem for theoretical physics in general [3], inflation has been a carefully developed paradigm with many explicit models. Unfortunately as far as inflationary model building is concerned, there are still many problems to be resolved. Particularly since many of the models suffer from super-Planckian VEV’s for the inflaton field [1], and therefore find themselves in a region where quantum gravity effects are non-negligible. -
Loop Quantum Cosmology, Modified Gravity and Extra Dimensions
universe Review Loop Quantum Cosmology, Modified Gravity and Extra Dimensions Xiangdong Zhang Department of Physics, South China University of Technology, Guangzhou 510641, China; [email protected] Academic Editor: Jaume Haro Received: 24 May 2016; Accepted: 2 August 2016; Published: 10 August 2016 Abstract: Loop quantum cosmology (LQC) is a framework of quantum cosmology based on the quantization of symmetry reduced models following the quantization techniques of loop quantum gravity (LQG). This paper is devoted to reviewing LQC as well as its various extensions including modified gravity and higher dimensions. For simplicity considerations, we mainly focus on the effective theory, which captures main quantum corrections at the cosmological level. We set up the basic structure of Brans–Dicke (BD) and higher dimensional LQC. The effective dynamical equations of these theories are also obtained, which lay a foundation for the future phenomenological investigations to probe possible quantum gravity effects in cosmology. Some outlooks and future extensions are also discussed. Keywords: loop quantum cosmology; singularity resolution; effective equation 1. Introduction Loop quantum gravity (LQG) is a quantum gravity scheme that tries to quantize general relativity (GR) with the nonperturbative techniques consistently [1–4]. Many issues of LQG have been carried out in the past thirty years. In particular, among these issues, loop quantum cosmology (LQC), which is the cosmological sector of LQG has received increasing interest and has become one of the most thriving and fruitful directions of LQG [5–9]. It is well known that GR suffers singularity problems and this, in turn, implies that our universe also has an infinitely dense singularity point that is highly unphysical. -
Aspects of Loop Quantum Gravity
Aspects of loop quantum gravity Alexander Nagen 23 September 2020 Submitted in partial fulfilment of the requirements for the degree of Master of Science of Imperial College London 1 Contents 1 Introduction 4 2 Classical theory 12 2.1 The ADM / initial-value formulation of GR . 12 2.2 Hamiltonian GR . 14 2.3 Ashtekar variables . 18 2.4 Reality conditions . 22 3 Quantisation 23 3.1 Holonomies . 23 3.2 The connection representation . 25 3.3 The loop representation . 25 3.4 Constraints and Hilbert spaces in canonical quantisation . 27 3.4.1 The kinematical Hilbert space . 27 3.4.2 Imposing the Gauss constraint . 29 3.4.3 Imposing the diffeomorphism constraint . 29 3.4.4 Imposing the Hamiltonian constraint . 31 3.4.5 The master constraint . 32 4 Aspects of canonical loop quantum gravity 35 4.1 Properties of spin networks . 35 4.2 The area operator . 36 4.3 The volume operator . 43 2 4.4 Geometry in loop quantum gravity . 46 5 Spin foams 48 5.1 The nature and origin of spin foams . 48 5.2 Spin foam models . 49 5.3 The BF model . 50 5.4 The Barrett-Crane model . 53 5.5 The EPRL model . 57 5.6 The spin foam - GFT correspondence . 59 6 Applications to black holes 61 6.1 Black hole entropy . 61 6.2 Hawking radiation . 65 7 Current topics 69 7.1 Fractal horizons . 69 7.2 Quantum-corrected black hole . 70 7.3 A model for Hawking radiation . 73 7.4 Effective spin-foam models . -
Is There Eternal Inflation in the Cosmic Landscape ?
Is there eternal inflation in the cosmic landscape ? Henry Tye Cornell University hep-th/0611148 ArXiv:0708.4374 [hep-th] with Qing-Guo Huang, ArXiv:0803.0663 [hep-th] with Dan Wohns and Yang Zhang, ArXiv:0811.3753 [hep-th] IPMU, 04/01/09 Expansion of the universe k ρm ρr H2 =Λ+ + + a2 a3 a4 • a(t) = the cosmic scale factor ~ size of universe • H = Hubble constant =(da/dt)/a • Λ = dark energy ~ cosmological constant ~ effective potential • k = curvature • ρm = matter density at initial time • ρr = radiation density at initial time • H = constant ⇒ a = eHt Inflation BRIEF ARTICLE THE AUTHOR 1 (1) d = s(Λc)/ξ +1 ∼ ∼ 1 ∼ −1/4 (2) ξ s(Λs) Λs ms (3) d>60 BRIEF ARTICLE (4) T (n) " T0/n THE AUTHOR 4 (5) Γ = msT (6) n ∼ 1/Hs 1 Eternal Inflation Ht 3 3Ht (7) (1) a(t) " e → V = a(t) " e τ > 1/H Suppose the universe is sitting at a local minimum, with a ln L (2)lifetime longer than the Hubble lntime:g ∼− L = −e Then the number of Hubble patches will increase −Si (3) exponentially. Even after some Hubble patchesαi have∼ e decayed, there would be many remaining Hubble patches (4) that continue to inflate. |βij| < αi (5) Eternal inflation impliesφi = thatϕi/f i somewhere in the universe (outside our horizon),d −1 (6) Γt ∼ n Γ0 inflation is still happening today. T (A → B)T (B → C) (7) T (A → C)= ∼ T0/2 T (A → B)+T (B → C) −S (8) ΓA→B = ΓB→C = Γ0 ∼ e 2 (9) ΓA→C ∼ ΓA→BΓB→C = Γ0 1 1 2 (10) tA→C = tA→B + tB→C = + ∼ → → 1 ΓA B ΓB C Γ0 Γ0 (11) Γ → = A C 2 −S (12) Γ(1) = Γ0 ∼ e − (13) Γ(2) ∼ e 2S − (14) Γ(2) ∼ e S − (15) Γ(n) ∼ e S (16) +H2φ2 2 2 (17) H = U/3MP 1 Flux compactification in Type II string theory where all moduli of the 6-dim. -
Abdus Salam United Nations Educational, Scientific and Cultural International XA0101583 Organization Centre
the 1(72001/34 abdus salam united nations educational, scientific and cultural international XA0101583 organization centre international atomic energy agency for theoretical physics NEW DIMENSIONS NEW HOPES Utpal Sarkar Available at: http://www.ictp.trieste.it/-pub-off IC/2001/34 United Nations Educational Scientific and Cultural Organization and International Atomic Energy Agency THE ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS NEW DIMENSIONS NEW HOPES Utpal Sarkar1 Physics Department, Visva Bharati University, Santiniketan 731235, India and The Abdus Salam Insternational Centre for Theoretical Physics, Trieste, Italy. Abstract We live in a four dimensional world. But the idea of unification of fundamental interactions lead us to higher dimensional theories. Recently a new theory with extra dimensions has emerged, where only gravity propagates in the extra dimension and all other interactions are confined in only four dimensions. This theory gives us many new hopes. In earlier theories unification of strong, weak and the electromagnetic forces was possible at around 1016 GeV in a grand unified theory (GUT) and it could get unified with gravity at around the Planck scale of 1019 GeV. With this new idea it is possible to bring down all unification scales within the reach of the next generation accelerators, i.e., around 104 GeV. MIRAMARE - TRIESTE May 2001 1 Regular Associate of the Abdus Salam ICTP. E-mail: [email protected] 1 Introduction In particle physics we try to find out what are the fundamental particles and how they interact. This is motivated from the belief that there must be some fundamental law that governs ev- erything. -
D-Branes in Topological Membranes
OUTP/03–21P HWM–03–14 EMPG–03–13 hep-th/0308101 August 2003 D-BRANES IN TOPOLOGICAL MEMBRANES P. Castelo Ferreira Dep. de Matem´atica – Instituto Superior T´ecnico, Av. Rovisco Pais, 1049-001 Lisboa, Portugal and PACT – University of Sussex, Falmer, Brighton BN1 9QJ, U.K. [email protected] I.I. Kogan Dept. of Physics, Theoretical Physics – University of Oxford, Oxford OX1 3NP, U.K. R.J. Szabo Dept. of Mathematics – Heriot-Watt University, Riccarton, Edinburgh EH14 4AS, U.K. [email protected] Abstract arXiv:hep-th/0308101v1 15 Aug 2003 It is shown how two-dimensional states corresponding to D-branes arise in orbifolds of topologically massive gauge and gravity theories. Brane vertex operators naturally appear in induced worldsheet actions when the three-dimensional gauge theory is minimally coupled to external charged matter and the orbifold relations are carefully taken into account. Boundary states corresponding to D-branes are given by vacuum wavefunctionals of the gauge theory in the presence of the matter, and their various constraints, such as the Cardy condition, are shown to arise through compatibility relations between the orbifold charges and bulk gauge invariance. We show that with a further conformally-invariant coupling to a dynamical massless scalar field theory in three dimensions, the brane tension is naturally set by the bulk mass scales and arises through dynamical mechanisms. As an auxilliary result, we show how to describe string descendent states in the three-dimensional theory through the construction of gauge-invariant excited wavefunctionals. Contents 1 INTRODUCTION AND SUMMARY 1 1.1 D-Branes .................................... -
Universit`A Degli Studi Di Padova
UNIVERSITA` DEGLI STUDI DI PADOVA Dipartimento di Fisica e Astronomia “Galileo Galilei” Corso di Laurea Magistrale in Fisica Tesi di Laurea Finite symmetry groups and orbifolds of two-dimensional toroidal conformal field theories Relatore Laureando Prof. Roberto Volpato Tommaso Macrelli Anno Accademico 2017/2018 Contents Introduction 5 1 Introduction to two dimensional Conformal Field Theory 7 1.1 The conformal group . .7 1.1.1 Conformal group in two dimensions . .9 1.2 Conformal invariance in two dimensions . 12 1.2.1 Fields and correlation functions . 12 1.2.2 Stress-energy tensor and conformal transformations . 13 1.2.3 Operator formalism: radial quantization . 14 1.3 General structure of a Conformal Field Theory in two dimensions . 16 1.3.1 Meromorphic Conformal Field Theory . 18 1.4 Examples . 22 1.4.1 Free boson . 22 1.4.2 Free Majorana fermion . 26 1.4.3 Ghost system . 27 2 Elements of String and Superstring Theory 28 2.1 Bosonic String Theory . 29 2.1.1 Classical Bosonic String . 29 2.1.2 Quantization . 31 2.1.3 BRST symmetry and Hilbert Space . 33 2.1.4 Spectrum of the Bosonic String . 34 2.1.5 What’s wrong with Bosonic String? . 36 2.2 Superstring Theory . 37 2.2.1 Introduction to Superstrings . 37 2.2.2 Heterotic String . 39 3 Compactifications of String Theory 41 3.1 An introduction: Kaluza-Klein compactification . 42 3.2 Free boson compactified on a circle . 43 3.2.1 Closed strings and T-Duality . 45 3.2.2 Enhanced symmetries at self-dual radius . -
Interactions and Forces
background sheet The Standard Model 2: Interactions and forces Force Interactions The Australian Curriculum refers to fundamental In any closed system a number of properties are forces, force-carrying particles and reactions between conserved. These include energy, momentum and particles. However in this resource we have chosen charge. Although the totals of each property are to use a terminology used by contemporary particle conserved, their distribution amongst components physicists, that of interactions. of a system can change. Whenever energy (or momentum, charge or any other conserved property) The difference between ‘force’ and ‘interaction’ is is redistributed amongst components of a system subtle, but significant. Understanding it helps make then an interaction has taken place. In other words, sense of this complex study area. interactions lead to redistribution of energy, Students were probably introduced to the topic momentum and charge. of force through ‘pushes and pulls’. They learnt In Figure 1 two particles change their motion as they that changes to an object’s motion didn’t happen approach. There has been an exchange of energy and spontaneously, but were the result of some external momentum between them, so an interaction has taken action: a push or a pull. place. In this case the interaction is a consequence Later on these ideas were codified in Newton’s laws of these particles having charge, so the interaction is of motion. Together with Newton’s universal law described as electromagnetic. of gravitation, and Coulomb’s law of electrostatic Physicists recognise four fundamental interactions: interaction, changes in motion of objects could be seen as a consequence of force-pairs (action and reaction) • gravitational interaction acting between two objects.