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Inflation, Large Branes, and the Shape of Space
Inflation, Large Branes, and the Shape of Space Brett McInnes National University of Singapore email: [email protected] ABSTRACT Linde has recently argued that compact flat or negatively curved spatial sections should, in many circumstances, be considered typical in Inflationary cosmologies. We suggest that the “large brane instability” of Seiberg and Witten eliminates the negative candidates in the context of string theory. That leaves the flat, compact, three-dimensional manifolds — Conway’s platycosms. We show that deep theorems of Schoen, Yau, Gromov and Lawson imply that, even in this case, Seiberg-Witten instability can be avoided only with difficulty. Using a specific cosmological model of the Maldacena-Maoz type, we explain how to do this, and we also show how the list of platycosmic candidates can be reduced to three. This leads to an extension of the basic idea: the conformal compactification of the entire Euclidean spacetime also has the topology of a flat, compact, four-dimensional space. arXiv:hep-th/0410115v2 19 Oct 2004 1. Nearly Flat or Really Flat? Linde has recently argued [1] that, at least in some circumstances, we should regard cosmological models with flat or negatively curved compact spatial sections as the norm from an Inflationary point of view. Here we wish to argue that cosmic holography, in the novel form proposed by Maldacena and Maoz [2], gives a deep new interpretation of this idea, and also sharpens it very considerably to exclude the negative case. This focuses our attention on cosmological models with flat, compact spatial sections. Current observations [3] show that the spatial sections of our Universe [as defined by observers for whom local isotropy obtains] are fairly close to being flat: the total density parameter Ω satisfies Ω = 1.02 0.02 at 95% confidence level, if we allow the imposition ± of a reasonable prior [4] on the Hubble parameter. -
Anomalies, Dualities, and Topology of D = 6 N = 1 Superstring Vacua
RU-96-16 NSF-ITP-96-21 CALT-68-2057 IASSNS-HEP-96/53 hep-th/9605184 Anomalies, Dualities, and Topology of D =6 N =1 Superstring Vacua Micha Berkooz,1 Robert G. Leigh,1 Joseph Polchinski,2 John H. Schwarz,3 Nathan Seiberg,1 and Edward Witten4 1Department of Physics, Rutgers University, Piscataway, NJ 08855-0849 2Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106-4030 3California Institute of Technology, Pasadena, CA 91125 4Institute for Advanced Study, Princeton, NJ 08540 Abstract We consider various aspects of compactifications of the Type I/heterotic Spin(32)/Z2 theory on K3. One family of such compactifications in- cludes the standard embedding of the spin connection in the gauge group, and is on the same moduli space as the compactification of arXiv:hep-th/9605184v1 25 May 1996 the heterotic E8 × E8 theory on K3 with instanton numbers (8,16). Another class, which includes an orbifold of the Type I theory re- cently constructed by Gimon and Polchinski and whose field theory limit involves some topological novelties, is on the moduli space of the heterotic E8 × E8 theory on K3 with instanton numbers (12,12). These connections between Spin(32)/Z2 and E8 × E8 models can be demonstrated by T duality, and permit a better understanding of non- perturbative gauge fields in the (12,12) model. In the transformation between Spin(32)/Z2 and E8 × E8 models, the strong/weak coupling duality of the (12,12) E8 × E8 model is mapped to T duality in the Type I theory. The gauge and gravitational anomalies in the Type I theory are canceled by an extension of the Green-Schwarz mechanism. -
2016 International Artist Exchanges' Creative
Photo: Laura Chichisan Why Support International Exchange among Artists? A Decade of Tracking the Economic, Cultural and Social Benefits of Doing So TransCultural Exchange’s Conferences on International Opportunities in the Arts Economic Impact Analysis and Program Evaluation 1 Why Support International Exchange among Artists? A Decade of Tracking the Economic, Cultural and Social Benefits of Doing So ______________________________________________________ Evaluation Staff Submitted by Carol Van Zandt/Mary Sherman Layout Carol Van Zandt/Siyi Yang Previous Surveys’ Research and Editing Support by Marie Costello, Tanya Gruenberger, Lindsay Ladner, Fahrin Zaman Online Survey Tool and Methodology Developed for TransCultural Exchange: Center for Policy Analysis at the University of Massachusetts Dartmouth TransCultural Exchange would like to thank the Massachusetts Cultural Council, Boston Cultural Council and National Endowment for the Arts for the funding to help produce this publication. Correspondence and inquiries should be addressed to: TransCultural Exchange The Artist Building at 300 Summer Street, #36 Boston, Massachusetts, 02210 617.670.0307 [email protected] 2 TransCultural Exchange’s Conferences on International Opportunities in the Arts Economic Impact Analysis and Program Evaluation Table of Contents FORWARD p.6 1.00 INTRODUCTION p.10 1.10 SUMMARY 2.00 ECONOMIC IMPACT AND SURVEY EVALUATION p.30 2.10 Methodology 2.11 Process Evaluation 2.12 Survey Evaluation 3.00 ECONOMIC IMPACT ANALYSIS p.32 3.10 Overview 3.11 -
Some Comments on Physical Mathematics
Preprint typeset in JHEP style - HYPER VERSION Some Comments on Physical Mathematics Gregory W. Moore Abstract: These are some thoughts that accompany a talk delivered at the APS Savannah meeting, April 5, 2014. I have serious doubts about whether I deserve to be awarded the 2014 Heineman Prize. Nevertheless, I thank the APS and the selection committee for their recognition of the work I have been involved in, as well as the Heineman Foundation for its continued support of Mathematical Physics. Above all, I thank my many excellent collaborators and teachers for making possible my participation in some very rewarding scientific research. 1 I have been asked to give a talk in this prize session, and so I will use the occasion to say a few words about Mathematical Physics, and its relation to the sub-discipline of Physical Mathematics. I will also comment on how some of the work mentioned in the citation illuminates this emergent field. I will begin by framing the remarks in a much broader historical and philosophical context. I hasten to add that I am neither a historian nor a philosopher of science, as will become immediately obvious to any expert, but my impression is that if we look back to the modern era of science then major figures such as Galileo, Kepler, Leibniz, and New- ton were neither physicists nor mathematicans. Rather they were Natural Philosophers. Even around the turn of the 19th century the same could still be said of Bernoulli, Euler, Lagrange, and Hamilton. But a real divide between Mathematics and Physics began to open up in the 19th century. -
2005 March Meeting Gears up for Showtime in the City of Angels
NEWS See Pullout Insert Inside March 2005 Volume 14, No. 3 A Publication of The American Physical Society http://www.aps.org/apsnews 2005 March Meeting Gears Up for Reborn Nicholson Medal Showtime in the City of Angels Stresses Mentorship Established in memory of Dwight The latest research relevance to the design R. Nicholson of the University of results on the spin Hall and creation of next- Iowa, who died tragically in 1991, effect, new chemistry generation nano-electro- and first given in 1994, the APS with superatoms, and mechanical systems Nicholson Medal has been reborn several sessions cel- (NEMS). Moses Chan this year as an award for human ebrating all things (Pennsylvania State Uni- outreach. According to the infor- Einstein are among the versity) will talk about mation contained on the Medal’s expected highlights at evidence of Bose-Einstein web site (http://www.aps.org/praw/ the 2005 APS March condensation in solid he- nicholso/index.cfm), the Nicholson meeting, to be held later lium, while Stanford Medal for Human Outreach shall Photo Credit: Courtesy of the Los Angeles Convention Center this month in Los University’s Zhixun Shen be awarded to a physicist who ei- Angeles, California. The will discuss how photo- ther through teaching, research, or Photo from Iowa University Relations. conference is the largest physics Boltzmann, and Ehrenfest, but also emission spectroscopy has science-related activities, Dwight R. Nicholson. meeting of the year, featuring some Emmy Noether, one of the rare emerged as a leading tool to push -
SUSY, Landscape and the Higgs
SUSY, Landscape and the Higgs Michael Dine Department of Physics University of California, Santa Cruz Workshop: Nature Guiding Theory, Fermilab 2014 Michael Dine SUSY, Landscape and the Higgs A tension between naturalness and simplicity There have been lots of good arguments to expect that some dramatic new phenomena should appear at the TeV scale to account for electroweak symmetry breaking. But given the exquisite successes of the Model, the simplest possibility has always been the appearance of a single Higgs particle, with a mass not much above the LEP exclusions. In Quantum Field Theory, simple has a precise meaning: a single Higgs doublet is the minimal set of additional (previously unobserved) degrees of freedom which can account for the elementary particle masses. Michael Dine SUSY, Landscape and the Higgs Higgs Discovery; LHC Exclusions So far, simplicity appears to be winning. Single light higgs, with couplings which seem consistent with the minimal Standard Model. Exclusion of a variety of new phenomena; supersymmetry ruled out into the TeV range over much of the parameter space. Tunings at the part in 100 1000 level. − Most other ideas (technicolor, composite Higgs,...) in comparable or more severe trouble. At least an elementary Higgs is an expectation of supersymmetry. But in MSSM, requires a large mass for stops. Michael Dine SUSY, Landscape and the Higgs Top quark/squark loop corrections to observed physical Higgs mass (A 0; tan β > 20) ≈ In MSSM, without additional degrees of freedom: 126 L 124 GeV H h m 122 120 4000 6000 8000 10 000 12 000 14 000 HMSUSYGeVL Michael Dine SUSY, Landscape and the Higgs 6y 2 δm2 = t m~ 2 log(Λ2=m2 ) H −16π2 t susy So if 8 TeV, correction to Higgs mass-squred parameter in effective action easily 1000 times the observed Higgs mass-squared. -
The Birth of String Theory
The Birth of String Theory Edited by Andrea Cappelli INFN, Florence Elena Castellani Department of Philosophy, University of Florence Filippo Colomo INFN, Florence Paolo Di Vecchia The Niels Bohr Institute, Copenhagen and Nordita, Stockholm Contents Contributors page vii Preface xi Contents of Editors' Chapters xiv Abbreviations and acronyms xviii Photographs of contributors xxi Part I Overview 1 1 Introduction and synopsis 3 2 Rise and fall of the hadronic string Gabriele Veneziano 19 3 Gravity, unification, and the superstring John H. Schwarz 41 4 Early string theory as a challenging case study for philo- sophers Elena Castellani 71 EARLY STRING THEORY 91 Part II The prehistory: the analytic S-matrix 93 5 Introduction to Part II 95 6 Particle theory in the Sixties: from current algebra to the Veneziano amplitude Marco Ademollo 115 7 The path to the Veneziano model Hector R. Rubinstein 134 iii iv Contents 8 Two-component duality and strings Peter G.O. Freund 141 9 Note on the prehistory of string theory Murray Gell-Mann 148 Part III The Dual Resonance Model 151 10 Introduction to Part III 153 11 From the S-matrix to string theory Paolo Di Vecchia 178 12 Reminiscence on the birth of string theory Joel A. Shapiro 204 13 Personal recollections Daniele Amati 219 14 Early string theory at Fermilab and Rutgers Louis Clavelli 221 15 Dual amplitudes in higher dimensions: a personal view Claud Lovelace 227 16 Personal recollections on dual models Renato Musto 232 17 Remembering the `supergroup' collaboration Francesco Nicodemi 239 18 The `3-Reggeon vertex' Stefano Sciuto 246 Part IV The string 251 19 Introduction to Part IV 253 20 From dual models to relativistic strings Peter Goddard 270 21 The first string theory: personal recollections Leonard Susskind 301 22 The string picture of the Veneziano model Holger B. -
Traversing Cosmological Singularities, Complete Journeys Through Spacetime Including Antigravity
Traversing Cosmological Singularities Complete Journeys Through Spacetime Including Antigravity ∗ Itzhak Bars Department of Physics and Astronomy, University of Southern California, Los Angeles, CA 90089-0484, USA A unique description of the Big Crunch-Big Bang transition is given at the classical gravity level, along with a complete set of homogeneous, isotropic, analytic solutions in scalar-tensor cosmology, with radiation and curvature. All solutions repeat cyclically; they have been obtained by using conformal gauge symmetry (Weyl symmetry) as a powerful tool in cosmology, and more generally in gravity. The significance of the Big Crunch-Big Bang transition is that it provides a model inde- pendent analytic resolution of the singularity, as an unambiguous and unavoidable solution of the equations at the classical gravitational physics level. It is controlled only by geometry (including anisotropy) and only very general features of matter coupled to gravity, such as kinetic energy of a scalar field, and radiation due to all forms of relativistic matter. This analytic resolution of the singularity is due to an attractor mechanism created by the leading terms in the cosmological equa- tion. It is unique, and it is unavoidable in classical relativity in a geodesically complete geometry. Its counterpart in quantum gravity remains to be understood. I. INTRODUCTION AND SUMMARY OF RESULTS Resolving the big bang singularity is one of the central challenges for fundamental physics and cosmology. The issue arises naturally in the context of classical relativity due to the geodesically incomplete nature of the singular spacetime [1]-[2]. The resolution may not be completed until the physics is understood in the context of quantum gravity. -
The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big
View metadata, citation and similar papers at core.ac.uk brought to you by CORE The Ekpyrotic Universe: Colliding Branes and the Origin ofprovided the by CERN Document Server Hot Big Bang Justin Khoury1,BurtA.Ovrut2,PaulJ.Steinhardt1 and Neil Turok 3 1 Joseph Henry Laboratories, Princeton University, Princeton, NJ 08544, USA 2 Department of Physics, University of Pennsylvania, Philadelphia, PA 19104-6396, USA 3 DAMTP, CMS, Wilberforce Road, Cambridge, CB3 0WA, UK Abstract We propose a cosmological scenario in which the hot big bang universe is produced by the collision of a brane in the bulk space with a bounding orb- ifold plane, beginning from an otherwise cold, vacuous, static universe. The model addresses the cosmological horizon, flatness and monopole problems and generates a nearly scale-invariant spectrum of density perturbations with- out invoking superluminal expansion (inflation). The scenario relies, instead, on physical phenomena that arise naturally in theories based on extra di- mensions and branes. As an example, we present our scenario predominantly within the context of heterotic M-theory. A prediction that distinguishes this scenario from standard inflationary cosmology is a strongly blue gravitational wave spectrum, which has consequences for microwave background polariza- tion experiments and gravitational wave detectors. Typeset using REVTEX 1 I. INTRODUCTION The Big Bang model provides an accurate account of the evolution of our universe from the time of nucleosynthesis until the present, but does not address the key -
Job Feldbrugge
Job Leon Feldbrugge University of Waterloo [email protected] Perimeter Institute http://www.perimeterinstitute.ca/personal/jfeldbrugge 31 Caroline Street North Waterloo ON N2L 2Y5, Canada Phone: (+1) 519-569-7600 x6610 Current position 2019 - present Postdoc at the Perimeter Institute (Canada) and Carnegie Mellon University (United States) Areas of specialization Theoretical astronomy • Theoretical cosmology: the early and late time universe • Mathematical physics Education 2015 - 2019 PHD Physics, Perimeter Institute, University of Waterloo Advisor: Neil Turok Thesis: Path integrals in the sky: Classical and quantum problems with minimal assumptions Defence date: October 17, 2019 2014 - 2015 MasteR Part III Mathematics (with distinction), University of Cambridge Committee: Paul Shellard and Tommaso Giannantonio Thesis: Primordial non-Gaussianity and large-scale structure 2012 - 2014 MasteR Physics (cum laude), van Swinderen Institute, University of Groningen 2012 - 2014 MasteR Astronomy (cum laude), Kapteyn Institute, University of Groningen 2012 - 2014 MasteR Mathematics (cum laude), Bernoulli Institute, University of Groningen Committee: Rien van de Weygaert (cosmology and large-scale structure formation) Diederik Roest (string cosmology) Aernout van Enter (statistical mechanics) Thesis: Statistics of caustics in large-scale structure formation 2009 - 2012 BacHeloR Physics (cum laude), van Swinderen Institute, University of Groningen 2009 - 2012 BacHeloR Astronomy (cum laude), Kapteyn Institute, University of Groningen -
Pos(HRMS)078 ∗ [email protected] Speaker
Two unforgettable years with Hector PoS(HRMS)078 Gabriele Veneziano∗ Collège de France, Paris, France and Theory Division, CERN, CH-1211 Geneva 23, Switzerland E-mail: [email protected] .......................... ........................... Quarks, Strings and the Cosmos - Hector Rubinstein Memorial Symposium August 09-11, 2010 AlbaNova (Stockholm) Sweden ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Two unforgettable years Gabriele Veneziano 1. Another lucky coincidence As a high school student in Florence I had the luck of being taught by some excellent teachers: Professor Tebaldo Liverani, in particular, was the one who initiated me to loving maths and physics. His preference, he once confessed, went to the former. However, after some hesitation, mine went to the latter as I entered the local University in 1960. Three years later I had to make another choice, this time about which branch of physics to go for. I was about to be "recruited" by the local high-energy experimental group when, just in time, Professor Raoul Gatto moved from Cagliari to Florence and "rescued" me to theoretical physics. PoS(HRMS)078 At the end of 1965 I received my "Laurea" in physics defending a thesis on some applications of the group SU(6)W . Only later I learned that the W in there apparently stood for Weizmann . Working in Florence as one of Gatto’s "gattini" was very stimulating. However, having always lived at home in my family in Florence, I felt the need to enlarge my horizons, both in physics and in life in general. -
Arxiv:0804.3210V1 [Hep-Ph] 20 Apr 2008 Nrdcint Tigter N Ag/Rvt Duality Gauge/Gravity and Theory String to Introduction ∗ † O Hs Tdnswihaesatn Olanqdadqpphysics View
Introduction to String Theory and Gauge/Gravity duality ∗ for students in QCD and QGP phenomenology Institut de Physique Th´eorique; URA 2306, unit´ede recherche associ´ee au CNRS, IPhT, CEA/Saclay, 91191 Gif-sur-Yvette Cedex, France Robi Peschanski † String theory has been initially derived from motivations coming from strong interaction phenomenology, but its application faced deep concep- tual and practical difficulties. The strong interactions found their the- oretical fundation elsewhere, namely on QCD, the quantum gauge field theory of quarks and gluons. Recently, the Gauge/Gravity correspondence allowed to initiate a reformulation of the connection between strings and gauge field theories, avoiding some of the initial drawbacks and opening the way to new insights on the gauge theory at strong coupling and even- tually QCD. Among others, the recent applications of the Gauge/Gravity correspondence to the formation of the QGP, the quark-gluon plasma, in heavy-ion reactions seem to provide a physically interesting insight on phe- nomenological features of the reactions. In these lectures we will give a arXiv:0804.3210v1 [hep-ph] 20 Apr 2008 simplified introduction to those aspects of string theory which, at the ori- gin and in the recent developments, are connected to strong interactions, for those students which are starting to learn QCD and QGP physics from an experimental or phenomenological point of view. PACS numbers: 11.15.-q,11.25.Tq ∗ Presented at the School on QCD, Low-x Physics and Diffraction, Copanello, Calabria, Italy, July 2007. † email:[email protected] (1) 2 proceedings printed on October 25, 2018 CONTENTS Lecture I: String Theory via Strong Interactions 1.