String Theory and Particle Physics: an Introuction to String Phenomenology Luis E
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TASI Lectures on String Compactification, Model Building
CERN-PH-TH/2005-205 IFT-UAM/CSIC-05-044 TASI lectures on String Compactification, Model Building, and Fluxes Angel M. Uranga TH Unit, CERN, CH-1211 Geneve 23, Switzerland Instituto de F´ısica Te´orica, C-XVI Universidad Aut´onoma de Madrid Cantoblanco, 28049 Madrid, Spain angel.uranga@cern,ch We review the construction of chiral four-dimensional compactifications of string the- ory with different systems of D-branes, including type IIA intersecting D6-branes and type IIB magnetised D-branes. Such models lead to four-dimensional theories with non-abelian gauge interactions and charged chiral fermions. We discuss the application of these techniques to building of models with spectrum as close as possible to the Stan- dard Model, and review their main phenomenological properties. We finally describe how to implement the tecniques to construct these models in flux compactifications, leading to models with realistic gauge sectors, moduli stabilization and supersymmetry breaking soft terms. Lecture 1. Model building in IIA: Intersecting brane worlds 1 Introduction String theory has the remarkable property that it provides a description of gauge and gravitational interactions in a unified framework consistently at the quantum level. It is this general feature (beyond other beautiful properties of particular string models) that makes this theory interesting as a possible candidate to unify our description of the different particles and interactions in Nature. Now if string theory is indeed realized in Nature, it should be able to lead not just to `gauge interactions' in general, but rather to gauge sectors as rich and intricate as the gauge theory we know as the Standard Model of Particle Physics. -
Lectures on D-Branes
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server CPHT/CL-615-0698 hep-th/9806199 Lectures on D-branes Constantin P. Bachas1 Centre de Physique Th´eorique, Ecole Polytechnique 91128 Palaiseau, FRANCE [email protected] ABSTRACT This is an introduction to the physics of D-branes. Topics cov- ered include Polchinski’s original calculation, a critical assessment of some duality checks, D-brane scattering, and effective worldvol- ume actions. Based on lectures given in 1997 at the Isaac Newton Institute, Cambridge, at the Trieste Spring School on String The- ory, and at the 31rst International Symposium Ahrenshoop in Buckow. June 1998 1Address after Sept. 1: Laboratoire de Physique Th´eorique, Ecole Normale Sup´erieure, 24 rue Lhomond, 75231 Paris, FRANCE, email : [email protected] Lectures on D-branes Constantin Bachas 1 Foreword Referring in his ‘Republic’ to stereography – the study of solid forms – Plato was saying : ... for even now, neglected and curtailed as it is, not only by the many but even by professed students, who can suggest no use for it, never- theless in the face of all these obstacles it makes progress on account of its elegance, and it would not be astonishing if it were unravelled. 2 Two and a half millenia later, much of this could have been said for string theory. The subject has progressed over the years by leaps and bounds, despite periods of neglect and (understandable) criticism for lack of direct experimental in- put. To be sure, the construction and key ingredients of the theory – gravity, gauge invariance, chirality – have a firm empirical basis, yet what has often catalyzed progress is the power and elegance of the underlying ideas, which look (at least a posteriori) inevitable. -
Pitp Lectures
MIFPA-10-34 PiTP Lectures Katrin Becker1 Department of Physics, Texas A&M University, College Station, TX 77843, USA [email protected] Contents 1 Introduction 2 2 String duality 3 2.1 T-duality and closed bosonic strings .................... 3 2.2 T-duality and open strings ......................... 4 2.3 Buscher rules ................................ 5 3 Low-energy effective actions 5 3.1 Type II theories ............................... 5 3.1.1 Massless bosons ........................... 6 3.1.2 Charges of D-branes ........................ 7 3.1.3 T-duality for type II theories .................... 7 3.1.4 Low-energy effective actions .................... 8 3.2 M-theory ................................... 8 3.2.1 2-derivative action ......................... 8 3.2.2 8-derivative action ......................... 9 3.3 Type IIB and F-theory ........................... 9 3.4 Type I .................................... 13 3.5 SO(32) heterotic string ........................... 13 4 Compactification and moduli 14 4.1 The torus .................................. 14 4.2 Calabi-Yau 3-folds ............................. 16 5 M-theory compactified on Calabi-Yau 4-folds 17 5.1 The supersymmetric flux background ................... 18 5.2 The warp factor ............................... 18 5.3 SUSY breaking solutions .......................... 19 1 These are two lectures dealing with supersymmetry (SUSY) for branes and strings. These lectures are mainly based on ref. [1] which the reader should consult for original references and additional discussions. 1 Introduction To make contact between superstring theory and the real world we have to understand the vacua of the theory. Of particular interest for vacuum construction are, on the one hand, D-branes. These are hyper-planes on which open strings can end. On the world-volume of coincident D-branes, non-abelian gauge fields can exist. -
Holography and Compactification
PUPT-1872 ITFA-99-14 Holography and Compactification Herman Verlinde Joseph Henry Laboratories, Princeton University, Princeton, NJ 08544 and Institute for Theoretical Physics, University of Amsterdam Valckenierstraat 65, 1018 XE Amsterdam Abstract arXiv:hep-th/9906182v1 24 Jun 1999 Following a recent suggestion by Randall and Sundrum, we consider string compactification scenarios in which a compact slice of AdS-space arises as a subspace of the compactifica- tion manifold. A specific example is provided by the type II orientifold equivalent to type I theory on (orbifolds of) T 6, upon taking into account the gravitational backreaction of the D3-branes localized inside the T 6. The conformal factor of the four-dimensional metric depends exponentially on one of the compact directions, which, via the holographic corre- spondence, becomes identified with the renormalization group scale in the uncompactified world. This set-up can be viewed as a generalization of the AdS/CFT correspondence to boundary theories that include gravitational dynamics. A striking consequence is that, in this scenario, the fundamental Planck size string and the large N QCD string appear as (two different wavefunctions of) one and the same object. 1 Introduction In string theory, when considered as a framework for unifying gravity and quantum mechan- ics, the fundamental strings are naturally thought of as Planck size objects. At much lower energies, such as the typical weak or strong interaction scales, the strings have lost all their internal structure and behave just as ordinary point-particles. The physics in this regime is therefore accurately described in terms of ordinary local quantum field theory, decoupled from the planckian realm of all string and quantum gravitational physics. -
Buffy & Angel Watching Order
Start with: End with: BtVS 11 Welcome to the Hellmouth Angel 41 Deep Down BtVS 11 The Harvest Angel 41 Ground State BtVS 11 Witch Angel 41 The House Always Wins BtVS 11 Teacher's Pet Angel 41 Slouching Toward Bethlehem BtVS 12 Never Kill a Boy on the First Date Angel 42 Supersymmetry BtVS 12 The Pack Angel 42 Spin the Bottle BtVS 12 Angel Angel 42 Apocalypse, Nowish BtVS 12 I, Robot... You, Jane Angel 42 Habeas Corpses BtVS 13 The Puppet Show Angel 43 Long Day's Journey BtVS 13 Nightmares Angel 43 Awakening BtVS 13 Out of Mind, Out of Sight Angel 43 Soulless BtVS 13 Prophecy Girl Angel 44 Calvary Angel 44 Salvage BtVS 21 When She Was Bad Angel 44 Release BtVS 21 Some Assembly Required Angel 44 Orpheus BtVS 21 School Hard Angel 45 Players BtVS 21 Inca Mummy Girl Angel 45 Inside Out BtVS 22 Reptile Boy Angel 45 Shiny Happy People BtVS 22 Halloween Angel 45 The Magic Bullet BtVS 22 Lie to Me Angel 46 Sacrifice BtVS 22 The Dark Age Angel 46 Peace Out BtVS 23 What's My Line, Part One Angel 46 Home BtVS 23 What's My Line, Part Two BtVS 23 Ted BtVS 71 Lessons BtVS 23 Bad Eggs BtVS 71 Beneath You BtVS 24 Surprise BtVS 71 Same Time, Same Place BtVS 24 Innocence BtVS 71 Help BtVS 24 Phases BtVS 72 Selfless BtVS 24 Bewitched, Bothered and Bewildered BtVS 72 Him BtVS 25 Passion BtVS 72 Conversations with Dead People BtVS 25 Killed by Death BtVS 72 Sleeper BtVS 25 I Only Have Eyes for You BtVS 73 Never Leave Me BtVS 25 Go Fish BtVS 73 Bring on the Night BtVS 26 Becoming, Part One BtVS 73 Showtime BtVS 26 Becoming, Part Two BtVS 74 Potential BtVS 74 -
Mathematically Talented Women in Hollywood: Fred in Angel
Mathematically Talented Women in Hollywood: Fred in Angel Sarah J. Greenwald and Jill E. Thomley Appalachian State University Introduction Individual faculty such as those represented in this volume have used popular culture in the class- room to alleviate math anxiety and to help students connect to significant mathematics. Recent educational initiatives such as We All Use Math Every Day [12], co-sponsored by CBS, Texas In- struments, and the National Council of Teachers of Mathematics, and MathMovesU [31], sponsored by Raytheon, strive to change attitudes and attract students to mathematics by capitalizing on student enjoyment of celebrities and popular culture. At the same time, Hollywood has increased its use of math and mathematicians, but some of those representations may not be all that positive for attracting students to mathematics. Others have examined the stereotype of the mentally ill mathematician (e.g., [25]), which may make it harder for students to identify with mathematicians. In this article we discuss the representations of mathematically talented women in Hollywood and provide a framework for examining the messages they may convey to the public and our students as we examine the example of physicist Fred Burkle in the television show Angel [1]. Unlike more recent representations of women mathematicians, such as Amita in NUMB3RS, which are aimed at a more mature audience, Angel aired on the WB network from October 1999 to May 2004 as part of a lineup of programs specifically targeted at teens and young adults. It is for this reason, and also because Fred’s experiences provide a rich context to discuss a variety of issues related to women in mathematics, that we chose Fred as a case study. -
University of Groningen Seven-Branes and Instantons In
University of Groningen Seven-branes and instantons in type IIB supergravity Hartong, Jelle IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2008 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Hartong, J. (2008). Seven-branes and instantons in type IIB supergravity. s.n. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 27-09-2021 Introduction The subject of this thesis will be introduced. The studies performed in the coming chapters attempt to improve on the understanding of certain aspects of string theory. Here, I will give a personal point of view on the subject of string theory after which I will briefly sketch the most elementary properties of string theory that allow me to further introduce the subject of this thesis. -
Non-Supersymmetric Ads and the Swampland
CALT-TH 2016-027, IPMU16-0139 Non-supersymmetric AdS and the Swampland Hirosi Ooguria,b and Cumrun Vafac a Walter Burke Institute for Theoretical Physics California Institute of Technology, Pasadena, CA 91125, USA b Kavli Institute for the Physics and Mathematics of the Universe University of Tokyo, Kashiwa, 277-8583, Japan c Center for the Fundamental Laws of Nature Harvard University, Cambridge, MA 02138, USA Abstract We propose to sharpen the weak gravity conjecture by the statement that, except for BPS states in a supersymmetric theory, the gravitational force is strictly weaker than any electric force and provide a number of evidences for this statement. Our conjecture implies that any non-supersymmetric anti-de Sitter vacuum supported by fluxes must be unstable, as is the case for all known attempts at such holographic constructions. arXiv:1610.01533v3 [hep-th] 25 Aug 2017 1 Introduction The weak gravity conjecture (WGC) [1] is an example of how seemingly consistent low energy gravitational theories can fail to have ultra-violet completion and instead belong to the swampland [2]; see [3] for more swampland constraints. Recently, there have been a number of papers checking and extending the WGC and applying it to cosmology [4–7,9–12]. The conjecture has also been related to the holographic principle in [13]. In this brief note, we propose sharpening of the WGC and point out that it implies that non-supersymmetric anti-de Sitter (AdS) vacua supported by fluxes are unstable. The WGC states that the mass of a particle carrying a basic unit of charge or its small multiple is less than or equal to that predicted if the particle were an extremal black hole. -
Lecture 1. Model Building in IIA: Intersecting Brane Worlds
Compactification, Model Building, and Fluxes Angel M. Uranga IFT, Madrid, and CERN, Geneva Lecture 1. Model building in IIA: Intersecting brane worlds We review the construction of chiral four-dimensional compactifications of type IIA string theory with intersecting D6-branes. Such models lead to four-dimensional the- ories with non-abelian gauge interactions and charged chiral fermions. We discuss the application of these techniques to building of models with spectrum as close as possible to the Standard Model, and review their main phenomenological properties. 1Introduction String theory has the remarkable property that it provides a description of gauge and gravitational interactions in a unified framework consistently at the quantum level. It is this general feature (beyond other beautiful properties of particular string models) that makes this theory interesting as a possible candidate to unify our description of the different particles and interactions in Nature. Now if string theory is indeed realized in Nature, it should be able to lead not just to ‘gauge interactions’ in general, but rather to gauge sectors as rich and intricate as the gauge theory we know as the Standard Model of Particle Physics. In these lecture we describe compactifications of string theory where sets of D-branes lead to gauge sectors close to the Standard Model. We furthermore discuss the interplay of such D-brane systems with flux compactifications, recently introduced to address the issues of moduli stabilization and supersymmetry breaking. Before starting, it is important to emphasize that there are other constructions in string theory which are candidates to reproduce the physics of the Standard Model at low energies, which do not involve D-branes. -
Supersymmetry Breaking Warped Throats and the Weak Gravity Conjecture Arxiv:1810.07673V4 [Hep-Th] 10 Apr 2019
IFT-UAM/CSIC-18-102 Supersymmetry Breaking Warped Throats and the Weak Gravity Conjecture Ginevra Buratti1, Eduardo Garc´ıa-Valdecasas1;2, Angel M. Uranga1 1 Instituto de F´ısicaTe´oricaIFT-UAM/CSIC, C/ Nicol´asCabrera 13-15, Campus de Cantoblanco, 28049 Madrid, Spain 2 Departamento de F´ısicaTe´orica,Facultad de Ciencias Universidad Aut´onomade Madrid, 28049 Madrid, Spain Abstract We generalize the swampland criterion forbidding stable non-supersymmetric AdS vacua and propose a new swampland conjecture forbidding stable non-supersymmetric \locally AdS" warped throats. The conjecture is motivated by the properties of systems of fractional D3- branes at singularities, and can be used to rule out large classes of warped throats with super- symmetry breaking ingredients, and their possible application to de Sitter uplift. In particular, this allows to reinterpret the runaway instabilities of the gravity dual of fractional branes in the dP1 theory, and to rule out warped throats with Dynamical Supersymmetry Breaking D-brane sectors at their bottom. We also discuss the instabilities of warped throats with supersymme- try broken by the introduction of anti-orientifold planes. These examples lead to novel decay arXiv:1810.07673v4 [hep-th] 10 Apr 2019 mechanisms in explicit non-supersymmetric examples of locally AdS warped throats, and also of pure AdS backgrounds. Contents 1 Introduction: Quantum Gravitational String Phenomenology1 2 Review of dimers and fractional branes3 3 The local AdS-WGC swampland criterion8 3.1 Derivation8 3.2 Evidence -
Recent Developments in Physics Far Beyond the Standard Model
FTUAM-99/02; IFT-UAM/CSIC-99-02 Recent Developments in Physics Far Beyond the Standard Model 1 L.E. Ib´a˜nez Departamento de F´ısica Te´orica C-XI and Instituto de F´ısica Te´orica C-XVI, Universidad Aut´onoma de Madrid Cantoblanco, 28049 Madrid, Spain Abstract String theory is the leading candidate for a unified theory of the standard model and gravity. In the last few years theorists have realized that there is a unique structure underlying string theory. In this unification a prominent role is played by the duality symmetries which relate different theories. I present a brief overview of these developements and discuss their possible impact in low-energy physics. One of the lessons learned is that the string scale, usually asumed to be of order of the Planck scale, could be arbitrarily low, even close to accelerator energies. arXiv:hep-ph/9901292v1 13 Jan 1999 1Contribution to the proceedings of the XXVI International Meeting on Fundamental Physics, La Toja, Spain (June 1998). 1 1 Far Beyond the Standard Model (FBSM) You have already heard many times that the Standard Model (SM) is fine and describes everything (except, maybe, neutrino masses) very well. And you have also heard almost the same number of times that in spite of that there are plenty of aspects of the SM that we do not yet understand. I am not going to repeat the well known list of questions without answers in the SM, it has not changed very much in the last decade. Instead of that I am going to talk today about one particular problem: the problem of combining the SM interactions with gravity. -
The Fayet-Iliopoulos Term in Type-I String Theory and M-Theory
IASSNS-HEP-97/128 CERN-TH/98-198 hep-ph/9806426 The Fayet-Iliop oulos term in Typ e-I string theory and M-theory 1 John March-Russell Scho ol of Natural Sciences Institute for Advanced Study Princeton, NJ 08540, USA and 2 Theoretical Physics Division CERN, CH-1211 Geneva 23, Switzerland Abstract The magnitude of the Fayet-Iliop oulos term is calculated for compacti ca- tions of Typ e-I string theory and Horava-Witten M-theory in which there exists a pseudo-anomalous U(1) . Contrary to various conjectures, it is found that X in leading order in the p erturbative expansion around the weakly-coupled M- theory or Typ e-I limits, a result identical to that of the weakly-coupled E E 8 8 heterotic string is obtained. The result is indep endent of the values chosen for the Typ e-I string scale or the size of the M-theory 11th dimension, only dep ending up on Newton's constant and the uni ed gauge coupling. 1 Research supp orted in part by U.S. Department of Energy contract #DE-FG02-90ER40542, and by the W.M. KeckFoundation. Alfred P. Sloan Foundation Fellow. 2 On leave of absence from the Institute for Advanced Study after June 2nd 1998. Email: [email protected] 1 Intro duction One of the most phenomenologically useful features of many string compacti cations is the existence of a U(1) symmetry with apparent eld theoretic anomalies [1]. These anomalies are cancelled by a four-dimensional version of the Green-Schwarz mecha- nism [2], whichinvolves shifts of the mo del indep endent axion of string theory under gauge and general co ordinate transformations.