The Ads5 × S5 Superstring
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Varying Fundamental Constants and Particle Physics
Varying fundamental constants and particle physics Rikard Enberg Tanumoy Mandal Uppsala Seminar, 2017-04-06 Overview • The general idea • Old idea: Varying electromagnetic coupling • Particle physics à new scalar particles • Generalization to SU(3) × SU(2) × U(1) • Generalization to Yukawa couplings • Collider signatures All results in this talk are based on work with Ulf Danielsson, Gunnar Ingelman, Tanumoy Mandal: arXiv:1601.00624 (Nucl. Phys. B, in press) and a forthcoming paper 2 Free parameters of the SM Fundamental constant: a parameter that cannot be explained by the theory (even in principle) How many parameters are there in the Standard Model? • 19: Yukawas, gauge couplings, CKM, theta, Higgs • 26: If we include neutrino mixing and masses • 27: If we include the cosmological constant • 31–37: If we add cosmological standard model [See e.g. Tegmark et al., PRD 73 (2006) 023505] And then there are c, ħ, G, kB, etc. … Recommended reading: R.N. Cahn, Rev. Mod. Phys. 68 (1996) 951-960 M.J. Duff, arXiv:1412.2040 3 From Wikipedia, “Standard Model” Wikipedia, “Standard From 4 What are the fundamental constants and what are just units? • There’s a debate in the literature about what are the fundamental constants, and how many are there. [e.g. Duff, Okun. Veneziano, arXiv:physics/0110060] • Michael Duff in particular argues that only dimensionless constants are fundamental. Dimensionful constants are just unit conversions (Fathoms and nautical miles) speed of light = 1 lightyear/year • “Asking whether c has varied over cosmic history … is like asking whether the number of litres to the gallon has varied” [M.J. -
Coordinate Space Approach to Double Copy Michael Duff Imperial College
Coordinate space approach to double copy Michael Duff Imperial College London based on [arXiv:1301.4176 arXiv:1309.0546 arXiv:1312.6523 arXiv:1402.4649 arXiv:1408.4434 arXiv:1602.08267 arXiv:1610.07192 arXiv:1707.03234 arXiv:1711.08476 arXiv:1807.02486 A. Anastasiou, L. Borsten, M. J. Duff, M. Hughes, A. Marrani, S. Nagy and M. Zoccali] Copenhagen August 2018 Basic idea Strong nuclear, Weak nuclear and Electromagnetic forces described by Yang-Mills gauge theory (non-abelian generalisation of Maxwell). Gluons, W, Z and photons have spin 1. Gravitational force described by Einstein’s general relativity. Gravitons have spin 2. But maybe (spin 2) = (spin 1)2. If so: 1) Do global gravitational symmetries follow from flat-space Yang-Mills symmetries? 2) Do local gravitational symmetries and Bianchi identities follow from flat-space Yang-Mills symmetries? 3) What about twin supergravities with same bosonic lagrangian but different fermions? 4) Are all supergravities Yang-Mills squared? Gravity as square of Yang-Mills A recurring theme in attempts to understand the quantum theory of gravity and appears in several different forms: Closed states from products of open states and KLT relations in string theory [Kawai, Lewellen, Tye:1985, Siegel:1988], On-shell D = 10 Type IIA and IIB supergravity representations from on-shell D = 10 super Yang-Mills representations [Green, Schwarz and Witten:1987], Vector theory of gravity [Svidzinsky 2009] Supergravity scattering amplitudes from those of super Yang-Mills in various dimensions, [Bern, Carrasco, Johanson:2008, 2010; Bern, Huang, Kiermaier, 2010: Bjerrum-Bohr, Damgaard, Monteiro, O’Connell 2012,Montiero, O’Connell, White 2011, 2014, Bianchi:2008, Elvang, Huang:2012, Cachazo:2013, Dolan:2013] Ambitwistor strings [Hodges:2011, Mason:2013, Geyer:2014] See talks by [Goldberger, Montiero, O’Connell] Gravity from Yang-Mills LOCAL SYMMETRIES: general covariance, local lorentz invariance, local supersymmetry, local p-form gauge invariance [ arXiv:1408.4434, Physica Scripta 90 (2015)] [ A. -
Abdus Salam United Nations Educational, Scientific and Cultural XA9952968 Organization International Centre
the IC/99/74 abdus salam united nations educational, scientific and cultural XA9952968 organization international centre international atomic energy agency for theoretical physics D = 4 YANG-MILLS CORRELATORS 5 FROM NSR STRINGS ON AdS5 x S Dimitri Polyakov 30-47 Available at: http://www.ictp.trieste.it/~pub-off IC/99/74 United Nations Educational Scientific and Cultural Organization and International Atomic Energy Agency THE ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS D = 4 YANG-MILLS CORRELATORS 5 FROM NSR STRINGS ON AdS5 x S Dimitri Polyakov^ The Abdus Salam International Centre for Theoretical Physics, Trieste, Italy. Abstract In our previous work (hep-th/9812044) we have proposed the sigma-model action, conjectured to be the NSR analogue of superstring theory on AdS$ x S5. This sigma- model is the NSR superstring action with potential term corresponding to the exotic 5- form vertex operator (branelike state). This 5-form potential plays the role of cosmological term, effectively curving the flat space-time geometry to that of AdS$ x S5. In this paper we study this ansatz in more detail and provide the derivation of the correlators of the four- dimensional super Yang-Mills theory from the above mentioned sigma-model. In particular, we show that the correlation function of two dilaton vertex operators in such a model reproduces the well-known result for the two-point function in N = 4 four-dimensional 2 2 super Yang-Mills theory: < F (x)F (y) >~ \JLy\» • MIRAMARE - TRIESTE July 1999 E-mail: [email protected] Introduction One of the most profound questions with regard to critical superstring theory in ten dimensions is its relation to our four-dimensional world. -
Brane Effective Actions, Kappa-Symmetry and Applications
Living Rev. Relativity, 15, (2012), 3 LIVINGREVIEWS http://www.livingreviews.org/lrr-2012-3 in relativity Brane Effective Actions, Kappa-Symmetry and Applications Joan Sim´on School of Mathematics, The University of Edinburgh, and Maxwell Institute for Mathematical Sciences Edinburgh EH9 3JZ, U.K. email: [email protected] Accepted on 9 January 2012 Published on 27 February 2012 Abstract This is a review on brane effective actions, their symmetries and some of their applications. Its first part covers the Green{Schwarz formulation of single M- and D-brane effective actions focusing on kinematical aspects: the identification of their degrees of freedom, the importance of world volume diffeomorphisms and kappa symmetry to achieve manifest spacetime covari- ance and supersymmetry, and the explicit construction of such actions in arbitrary on-shell supergravity backgrounds. Its second part deals with applications. First, the use of kappa symmetry to determine supersymmetric world volume solitons. This includes their explicit construction in flat and curved backgrounds, their interpretation as Bogomol'nyi{Prasad–Sommerfield (BPS) states carrying (topological) charges in the supersymmetry algebra and the connection between su- persymmetry and Hamiltonian BPS bounds. When available, I emphasise the use of these solitons as constituents in microscopic models of black holes. Second, the use of probe approx- imations to infer about the non-trivial dynamics of strongly-coupled gauge theories using the anti de Sitter/conformal field theory (AdS/CFT) correspondence. This includes expectation values of Wilson loop operators, spectrum information and the general use of D-brane probes to approximate the dynamics of systems with small number of degrees of freedom interacting with larger systems allowing a dual gravitational description. -
Introduction to Path Integral Methods in String Theory
Introduction to path integral methods in string theory Sergio Ernesto Aguilar Guti´errez1 1Instituto de F´ısica Te´orica, Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271, 01140-070 S~aoPaulo, SP, Brazil∗ (Dated: November 30, 2018) Contents I. Introduction 1 II. Functional methods in bosonic string theory 2 A. Polyakov action 2 B. Symmetries 3 C. Equations of motion and boundary conditions 4 D. Polyakov path integral 6 E. BRST quantization 10 F. Representation theory 11 III. Functional methods in the RNS formalism 12 A. Superstring theory in the RNS formalism 12 B. R and NS sectors 14 C. Local symmetries of the action 16 D. Path integrals in RNS 17 References 19 I. INTRODUCTION The fundamentals of path integral methods in string theory are reviewed with emphasis in the development of the Faddeev Popov ghost that emerge from overcounting of configurations and the conditions that the string theory requires for maintaining Weyl invariance. Since the lecture is presented for a course that does not assume previous knowledge in string theory, I include an introduction to both bosonic and superstring theory (in the RNS formalism). This text begins with an introduction to bosonic string theory, we study the symmetries of the Polyakov action, we work out the canonical quantization of the theory to calculate its central charge. Later the path integral formulation is introduced with the appearance of Faddeev-Popov ghosts, we consider their canonical quantization for computing the central charge. The total central charge generates an anomaly in the Weyl invariance of the theory. The vanishing of such term has powerful implications that yield conditions related with the possible physical states and the dimensions of the theory. -
Quantum Gravity: a Primer for Philosophers∗
Quantum Gravity: A Primer for Philosophers∗ Dean Rickles ‘Quantum Gravity’ does not denote any existing theory: the field of quantum gravity is very much a ‘work in progress’. As you will see in this chapter, there are multiple lines of attack each with the same core goal: to find a theory that unifies, in some sense, general relativity (Einstein’s classical field theory of gravitation) and quantum field theory (the theoretical framework through which we understand the behaviour of particles in non-gravitational fields). Quantum field theory and general relativity seem to be like oil and water, they don’t like to mix—it is fair to say that combining them to produce a theory of quantum gravity constitutes the greatest unresolved puzzle in physics. Our goal in this chapter is to give the reader an impression of what the problem of quantum gravity is; why it is an important problem; the ways that have been suggested to resolve it; and what philosophical issues these approaches, and the problem itself, generate. This review is extremely selective, as it has to be to remain a manageable size: generally, rather than going into great detail in some area, we highlight the key features and the options, in the hope that readers may take up the problem for themselves—however, some of the basic formalism will be introduced so that the reader is able to enter the physics and (what little there is of) the philosophy of physics literature prepared.1 I have also supplied references for those cases where I have omitted some important facts. -
Introduction to Superstring Theory
Introduction to Superstring Theory Carmen N´u~nez IAFE (UBA-CONICET) & PHYSICS DEPT. (University of Buenos Aires) VI ICTP LASS 2015 Mexico, 26 October- 6 November 2015 . Programme Class 1: The classical fermionic string Class 2: The quantized fermionic string Class 3: Partition Function Class 4: Interactions . Outline Class 1: The classical fermionic string The action and its symmetries Gauge fixing and constraints Equations of motion and boundary conditions Oscillator expansions . The spectra of bosonic strings contain a tachyon ! it might indicate the vacuum has been incorrectly identified. The mass squared of a particle T is the quadratic term in the 2 @2V (T ) j − 4 ) action: M = @T 2 T =0 = α0 = we are expanding around a maximum of V . If there is some other stable vacuum, this is not an actual inconsistency. Why superstrings? . The mass squared of a particle T is the quadratic term in the 2 @2V (T ) j − 4 ) action: M = @T 2 T =0 = α0 = we are expanding around a maximum of V . If there is some other stable vacuum, this is not an actual inconsistency. Why superstrings? The spectra of bosonic strings contain a tachyon ! it might indicate the vacuum has been incorrectly identified. If there is some other stable vacuum, this is not an actual inconsistency. Why superstrings? The spectra of bosonic strings contain a tachyon ! it might indicate the vacuum has been incorrectly identified. The mass squared of a particle T is the quadratic term in the 2 @2V (T ) j − 4 ) action: M = @T 2 T =0 = α0 = we are expanding around a maximum of V . -
String Theory and Our Relationship with Nature: the Convergence of Science, Curriculum Theory, and the Environment
Georgia Southern University Digital Commons@Georgia Southern Electronic Theses and Dissertations Graduate Studies, Jack N. Averitt College of Fall 2010 String Theory and Our Relationship with Nature: The Convergence of Science, Curriculum Theory, and the Environment Virginia Therese Bennett Follow this and additional works at: https://digitalcommons.georgiasouthern.edu/etd Recommended Citation Bennett, Virginia Therese, "String Theory and Our Relationship with Nature: The Convergence of Science, Curriculum Theory, and the Environment" (2010). Electronic Theses and Dissertations. 530. https://digitalcommons.georgiasouthern.edu/etd/530 This dissertation (open access) is brought to you for free and open access by the Graduate Studies, Jack N. Averitt College of at Digital Commons@Georgia Southern. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of Digital Commons@Georgia Southern. For more information, please contact [email protected]. STRING THEORY AND OUR RELATIONSHIP WITH NATURE: THE CONVERGENCE OF SCIENCE, CURRICULUM THEORY, AND THE ENVIRONMENT by VIRGINIA THERESE BENNETT (Under the Direction of John A. Weaver) ABSTRACT Curriculum Theory affords us the opportunity to examine education from a multitude of directions. This work takes advantage of that opportunity to explore the relationships between science, nature, and curriculum using string theory and our ideas about the environment as a backdrop. Both the energy and multiple possibilities created by strings and the rich history leading up to the theory help to illustrate the many opportunities we have to advance discussions in alternative ways of looking at science. By considering the multiple dimensions inherent in string theory as multiple pathways and interweaving metaphors from Deleuze and Guattari, Michel Serres, and Donna Haraway, our approach to environmental issues and environmental education allow us to include alternative ways of looking at the world. -
String Theory and M-Theory: a Modern Introduction Katrin Becker, Melanie Becker, and John H
Cambridge University Press 978-0-521-86069-7 - String Theory and M-Theory: A Modern Introduction Katrin Becker, Melanie Becker, and John H. Schwarz Frontmatter More information STRING THEORY AND M-THEORY A MODERN INTRODUCTION String theory is one of the most exciting and challenging areas of modern theoretical physics. This book guides the reader from the basics of string theory to very recent developments at the frontier of string theory research. The book begins with the basics of perturbative string theory, world-sheet supersymmetry, space-time supersymmetry, conformal field theory and the heterotic string, and moves on to describe modern developments, including D-branes, string dualities and M-theory. It then covers string geometry (including Calabi–Yau compactifications) and flux compactifications, and applications to cosmology and particle physics. One chapter is dedicated to black holes in string theory and M-theory, and the microscopic origin of black-hole entropy. The book concludes by presenting matrix theory, AdS/CFT duality and its generalizations. This book is ideal for graduate students studying modern string theory, and it will make an excellent textbook for a 1-year course on string theory. It will also be useful for researchers interested in learning about developments in modern string theory. The book contains about 120 solved exercises, as well as about 200 homework problems, solutions of which are available for lecturers on a pass- word protected website at www.cambridge.org/9780521860697. K ATRIN B ECKER is a Professor of physics at Texas A & M University. She was awarded the Radcliffe Fellowship from Harvard University in 2006 and received the Alfred Sloan Fellowship in 2003. -
Constellations Education Resource Pack
CONSTELLATIONS BACKGROUND RESOURCES CONTENTS 1. About the Production 2. About the Writer 3. About the Play 4 & 5. Interview with Nick Payne 6. Interview with Lucy Cullingford 7. Practical Activities 8. Scene Study 9. Further Reading and Education at The Royal Court These resources are intended to give teachers and students a detailed insight into the creative process behind developing and staging Constellations. Through interviews, production notes and rehearsal techniques, they demonstrate how the writer, director and cast worked in collaboration to create the show. We aim to provide useful information and opportunities to help students discover the unique world of the play for themselves. DUKE OF YORKS THEATRE Constellations by Nick Payne Constellations had its premier at The Royal Court Jerwood Downstairs on Friday 13th January 2012 Constellations had its premier at The Duke of Yorks Theatre on Friday 9th November 2012 by Nick Payne Marianne Sally Hawkins Roland Rafe Spall Director Michael Longhurst Designer Tom Scutt Lighting Designer Lee Curran Composer Simon Slater Sound Designer David McSeveney Casting Director Amy Ball Assistant Director Sam Caird Production Manager Tariq Rifaat Movement Director Lucy Cullingford BSLBT Consultant Daryl Jackson Fight Director Kate Waters Stage Managers Rhiannon Harper, Bryan Paterson Stage Management Work Placement Amy Burkett Costume Supervisor Iona Kenrick WHAT THE CRITICS SAY: “Payne announced himself as a dramatist of rich humanity, vitality and promise. Here he makes a quantum leap with a -
Arxiv:1701.02422V1 [Hep-Th] 10 Jan 2017 Asnmes 46.M 11.15.Bt 04.60.-M, Numbers: PACS Operators
UCLA/16/TEP/103 SLAC–PUB–16905 Two-Loop Renormalization of Quantum Gravity Simplified Zvi Berna, Huan-Hang Chib, Lance Dixonb and Alex Edisona aMani L. Bhaumik Institute for Theoretical Physics Department of Physics and Astronomy University of California at Los Angeles Los Angeles, CA 90095, USA bSLAC National Accelerator Laboratory Stanford University Stanford, CA 94309, USA Abstract The coefficient of the dimensionally regularized two-loop R3 divergence of (nonsupersymmetric) gravity theories has recently been shown to change when non-dynamical three forms are added to the theory, or when a pseudo-scalar is replaced by the anti-symmetric two-form field to which it is dual. This phenomenon involves evanescent operators, whose matrix elements vanish in four dimensions, including the Gauss-Bonnet operator which is also connected to the trace anomaly. On the other hand, these effects appear to have no physical consequences in renormalized scattering arXiv:1701.02422v1 [hep-th] 10 Jan 2017 processes. In particular, the dependence of the two-loop four-graviton scattering amplitude on the renormalization scale is simple. In this paper, we explain this result for any minimally-coupled massless gravity theory with renormalizable matter interactions by using unitarity cuts in four dimensions and never invoking evanescent operators. PACS numbers: 04.60.-m, 11.15.Bt 1 I. INTRODUCTION Recent results show that the ultraviolet structure of gravity is much more interesting and subtle than might be anticipated from standard considerations. One example of a new ultraviolet surprise is the recent identification of “enhanced ultraviolet cancellations” in certain supergravity theories [1, 2], which are as yet unexplained by standard symme- tries [3]. -
Heterotic String Theory on Calabi-Yau - Manifolds in the Green-Schwarz Formalism*
1 . SLAC - PUB - 4071 August 1986 -. T HETEROTIC STRING THEORY ON CALABI-YAU - MANIFOLDS IN THE GREEN-SCHWARZ FORMALISM* ASHOKE SEN Stanford Linear Accelerator Center - Stanford University, Stanford, California, 94305 ABSTRACT The a-model describing the propagation of the heterotic string in a Calabi- Yau background is written down in the Green-Schwarz formulation. This model has manifest N=l space-time supersymmetry, however only the SO(2) subgroup - of the four dimensional Lorentz group is realized linearly. The criteria for the existence of the full SO(3,l) L orentz symmetry in this model are studied. These requirements turn out to be identical to those obtained by demanding the exis- =- tence of space-time supersymmetry in the Neveu-Schwarz-Ramond formulation - of the theory, where the SO(3,l) L orentz symmetry is manifest, but space-time supersymmetry is not. The analysis is easily generalized to more general back- grounds, which give rise to (2,0) su p erconformal field theories on the world sheet. Finally it is shown that if the requirements which give unbroken N=l space-time supersymmetry and full SO(3,l) L orentz invariance are satisfied, then the unbro- ken gauge group after the compactification of the &3 x J?& heterotic string theory on Calabi-Yau spaces iS Es X Es. - Submitted to Nuclear Physics B * Work supported by the Department of Energy, contract DE - AC03 - 76SF00515. 1. INTRODUCTION Current interest in string theories has its origin at the discovery of anomaly cancellation,[ll subsequent discovery of the heterotic string theory, 121and the -- - semi-realistic compactification of this theory on Calabi-Yau manifolds PI and orbifolds.