Abelian Gauge Symmetries in F-Theory and Dual Theories

Total Page:16

File Type:pdf, Size:1020Kb

Abelian Gauge Symmetries in F-Theory and Dual Theories University of Pennsylvania ScholarlyCommons Publicly Accessible Penn Dissertations 2016 Abelian Gauge Symmetries in F-Theory and Dual Theories Peng Song University of Pennsylvania, [email protected] Follow this and additional works at: https://repository.upenn.edu/edissertations Part of the Mathematics Commons, and the Physics Commons Recommended Citation Song, Peng, "Abelian Gauge Symmetries in F-Theory and Dual Theories" (2016). Publicly Accessible Penn Dissertations. 2031. https://repository.upenn.edu/edissertations/2031 This paper is posted at ScholarlyCommons. https://repository.upenn.edu/edissertations/2031 For more information, please contact [email protected]. Abelian Gauge Symmetries in F-Theory and Dual Theories Abstract In this dissertation, we focus on important physical and mathematical aspects, especially abelian gauge symmetries, of F-theory compactifications and its dual formulations within type IIB and heterotic string theory. F-theory is a non-perturbative formulation of type IIB string theory which enjoys important dualities with other string theories such as M-theory and E8 × E8 heterotic string theory. One of the main strengths of F-theory is its geometrization of many physical problems in the dual string theories. In particular, its study requires a lot of mathematical tools such as advanced techniques in algebraic geometry. Thus, it has also received a lot of interests among mathematicians, and is a vivid area of research within both the physics and the mathematics community. Although F-theory has been a long-standing theory, abelian gauge symmetry in Ftheory has been rarely studied, until recently. Within the mathematics community, in 2009, Grassi and Perduca first discovered the possibility of constructing elliptically fibered varieties with non-trivial toric Mordell-Weil group. In the physics community, in 2012, Morrison and Park first made a major advancement by constructing general F-theory compactifications with U(1) abelian gauge symmetry. They found that in such cases, the ellipticallyfibered Calabi-Yau manifold that F-theory needs to be compactified on has its fiber being a generic elliptic curve in the blow-up of the weighted projective space P(1;1;2) at one point. Subsequent developments have been made by Cvetiˇc, Klevers and Piragua extended the works of Morrison and Park and constructed general F-theory compactifications with U(1) U(1) abelian gauge symmetry. They found that in the U(1) × U(1) abelian gauge symmetry case, the elliptically-fibered Calabi-Yau manifold that F-theory needs to be compactified on has its fiber being a generic elliptic curve in the del Pezzo surface dP2. In chapter 2 of this dissertation, I bring this a step further by constructing general F-theory compactifications with U(1) × U(1) × U(1) abelian gauge symmetry. I showed that in the case with three U(1) factors, the general elliptic fiber is a complete intersection of two quadrics in P3, and the general elliptic fiber in the fully esolvr ed elliptic fibration is embedded as the generic Calabi-Yau complete intersection into Bl3P3, the blow-up of P3 at three generic points. This eventually leads to our analysis of representations of massless matter at codimension two singularities of these compactifications. Interestingly, we obtained a tri-fundamental representation which is unexpected from perturbative Type II compactifications, further illustrating the power of F-theory. In chapter 1 of this dissertation, I proved finiteness of a egionr of the string landscape in Type IIB compactifications. String compactifications give rise to a collection of effective low energy theories, known as the string landscape. However, it is not known whether the number of physical theories we can derive from the string landscape is finite. The vastness of the string landscape also poses a serious challenge to attempts of studying it. A breakthrough was made by Douglas and Taylor in 2007 when they studied the landscape of intersecting brane models in Type IIA compactifications on a particular Z2× Z2 orientifold. They found that two consistency conditions, namely the D6-brane tadpole cancellation condition, and the conditions on D6-branes that were required for N = 1 supersymmetry in four dimensions, only permitted a finite number of D6-brane configurations. These finite number of allowed D6-brane configurations thus result in only a finite number of gauge sectors in a 4D supergravity theory, allowing them to be studied explicitly. Douglas and Taylor also believed that the phenomenon of using tadpole cancellation and supersymmetry consistency conditions to restrict the possible number of allowed configurations to a finite one is not a mere coincidence unique to their construction; they conjectured that this phenomenon also holds for theories with magnetised D9- or D5-branes compactified on elliptically fibered Calabi-Yau threefolds. Indeed, this was what my collaborators and I also felt. To this end, I showed, using a mathematical proof, that their conjecture is indeed true for elliptically fibered Calabi-Yau threefolds p X B whose base B satisfy a few easily-checked conditions (summarized in chapter 1 of this dissertation). In particular, these conditions are satisfied by, although not limited to, the almost Fano twofold bases B given by the toric varieties associated to all 16 reflexive two-dimensional polytopes and the del Pezzo surfaces dPn for n = 0;1; :::; 8. This list, in particular, also includes the Hirzebruch surfaces F0 = P1 ×P1;F1 = dP1;F2. My proof also allowed us to derive the explicit and computable bounds on all flux quanta and on the number of D5-branes. These bounds only depends on the topology of the base B and are independent on the continuous moduli of the compactification, in particular the Kahler moduli, as long as the supergravity approximation is valid. Physically, my proof showed that these compactifications only give rise to a finite number of four-dimensional N = 1 supergravity theories, and that these theories only have finitely many gauge sectors with finitely many chiral spectra. Such finiteness properties are not observed in generic quantum field theories, further fortifying superstring theory as a more promising theory. In chapter 3 of this dissertation, I study abelian gauge symmetries in the duality between F-theory and E8 × E8 heterotic string theory. It is conjectured that F-theory, when compactified on an elliptic K3-fibered (n + 1)-dimensional Calabi-Yau manifold X B, and heterotic string theory when compactified on an elliptically fibered n-dimensional Calabi-Yau manifold Z B with the same base B, are dual to each other. Thus under such duality, in particular, if the F-theory compactification admits abelian gauge symmetries, the dual heterotic string theory must admit the same abelian gauge symmetry as well. However, how abelian gauge symmetries can arise in the dual heterotic string theory has never been studied. The main goal of this chapter is to study exactly this. We start with F-theory compactifications with abelian gauge symmetry. With the help of a mathematical lemma as well as a computer code that I came up with, I was able to construct a rich list of specialized examples with specific abelian and nonabelian gauge groups on the F-theory side. The computer code also directly computes spectral cover data for each example constructed, allowing us to further analyze how abelian gauge symmetries arise on heterotic side. Eventually, we found that in general, there are three ways in which U(1)-s can arise on the heterotic side: the case where the heterotic theory admits vector bundles with S(U(1) ×U(m)) structure group, the case where the heterotic theory admits vector bundles with SU(m)×Zn structure group, as well as the case where the heterotic theory admits vector bundles with structure groups having a centralizer in E8 which contains a U(1) factor. Another important achievement was my discovery of the non-commutativity of the semi-stable degeneration map which splits a K3 surface into two half K3 surfaces, and the map to Weierstrass form, which was not previously known in the literature. Degree Type Dissertation Degree Name Doctor of Philosophy (PhD) Graduate Group Physics & Astronomy First Advisor Mirjam Cvetic Keywords abelian gauge theory, algebraic geometry, F-theory, string compactification, string landscape Subject Categories Mathematics | Physics This dissertation is available at ScholarlyCommons: https://repository.upenn.edu/edissertations/2031 ABELIAN GAUGE SYMMETRIES IN F-THEORY AND DUAL THEORIES Peng Song A DISSERTATION in Physics and Astronomy Presented to the Faculties of the University of Pennsylvania in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy 2016 Mirjam Cvetic,ˇ Professor of Physics and Astronomy Supervisor of Dissertation Philip Nelson, Professor of Physics and Astronomy Graduate Group Chairperson Dissertation Committee Mirjam Cvetic,ˇ Professor of Physics and Astronomy Antonella Grassi, Professor of Mathematics Elliot Lipeles, Professor of Physics and Astronomy Philip Nelson, Professor of Physics and Astronomy Evelyn Thomson, Professor of Physics and Astronomy ABELIAN GAUGE SYMMETRIES IN F-THEORY AND DUAL THEORIES COPYRIGHT 2016 Peng Song ACKNOWLEDGMENTS This dissertation would not have been possible without the support of my family, my advi- sor, my research group and my good friends. First and foremost, I want to thank my family for being so supportive and understand- ing. It is their morale support that fuelled me to move on throughout these years. Next, I would like to thank my advisor Mirjam Cvetic,ˇ for her constant guidance in my pursuit of physics and mathematics. Her keen insights and intuitions have always shed light on the obscurities I encountered during my research works. There were many occasions in which Professor Cveticˇ have successfully solved problems using innovative and creative approaches that no one else in my group thought of, creating important breakthroughs. I am extremely grateful to the great mathematician Ron Donagi, from whom I learnt a great deal of mathematics and physics.
Recommended publications
  • A String Landscape Perspective on Naturalness Outline • Preliminaries
    A String Landscape Perspective on Naturalness A. Hebecker (Heidelberg) Outline • Preliminaries (I): The problem(s) and the multiverse `solution' • Preliminaries (II): From field theory to quantum gravity (String theory in 10 dimensions) • Compactifications to 4 dimensions • The (flux-) landscape • Eternal inflation, multiverse, measure problem The two hierarchy/naturalness problems • A much simplified basic lagrangian is 2 2 2 2 4 L ∼ MP R − Λ − jDHj + mhjHj − λjHj : • Assuming some simple theory with O(1) fundamental parameters at the scale E ∼ MP , we generically expectΛ and mH of that order. • For simplicity and because it is experimentally better established, I will focus in on theΛ-problem. (But almost all that follows applies to both problems!) The multiverse `solution' • It is quite possible that in the true quantum gravity theory, Λ comes out tiny as a result of an accidental cancellation. • But, we perceive that us unlikely. • By contrast, if we knew there were 10120 valid quantum gravity theories, we would be quite happy assuming that one of them has smallΛ. (As long as the calculations giving Λ are sufficiently involved to argue for Gaussian statisics of the results.) • Even better (since in principle testable): We could have one theory with 10120 solutions with differentΛ. Λ-values ! The multiverse `solution' (continued) • This `generic multiverse logic' has been advertised long before any supporting evidence from string theory existed. This goes back at least to the 80's and involves many famous names: Barrow/Tipler , Tegmark , Hawking , Hartle , Coleman , Weinberg .... • Envoking the `Anthropic Principle', [the selection of universes by demanding features which we think are necessary for intelligent life and hence for observers] it is then even possible to predict certain observables.
    [Show full text]
  • String Theory for Pedestrians
    String Theory for Pedestrians – CERN, Jan 29-31, 2007 – B. Zwiebach, MIT This series of 3 lecture series will cover the following topics 1. Introduction. The classical theory of strings. Application: physics of cosmic strings. 2. Quantum string theory. Applications: i) Systematics of hadronic spectra ii) Quark-antiquark potential (lattice simulations) iii) AdS/CFT: the quark-gluon plasma. 3. String models of particle physics. The string theory landscape. Alternatives: Loop quantum gravity? Formulations of string theory. 1 Introduction For the last twenty years physicists have investigated String Theory rather vigorously. Despite much progress, the basic features of the theory remain a mystery. In the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics (QCD)– a theory of quarks and gluons – and despite their early promise, strings faded away. This time string theory is a credible candidate for a theory of all interactions – a unified theory of all forces and matter. Additionally, • Through the AdS/CFT correspondence, it is a valuable tool for the study of theories like QCD. • It has helped understand the origin of the Bekenstein-Hawking entropy of black holes. • Finally, it has inspired many of the scenarios for physics Beyond the Standard Model of Particle physics. 2 Greatest problem of twentieth century physics: the incompatibility of Einstein’s General Relativity and the principles of Quantum Mechanics. String theory appears to be the long-sought quantum mechanical theory of gravity and other interactions. It is almost certain that string theory is a consistent theory. It is less certain that it describes our real world.
    [Show full text]
  • The String Theory Landscape and Cosmological Inflation
    The String Theory Landscape and Cosmological Inflation Background Image: Planck Collaboration and ESA The String Theory Landscape and Cosmological Inflation Outline • Preliminaries: From Field Theory to Quantum Gravity • String theory in 10 dimensions { a \reminder" • Compactifications to 4 dimensions • The (flux-) landscape • Eternal inflation and the multiverse • Slow-roll inflation in our universe • Recent progress in inflation in string theory From Particles/Fields to Quantum Gravity • Naive picture of particle physics: • Theoretical description: Quantum Field Theory • Usually defined by an action: Z 4 µρ νσ S(Q)ED = d x Fµν Fρσ g g with T ! @Aµ @Aν 0 E Fµν = − = @xν @xµ −E "B Gravity is in principle very similar: • The metric gµν becomes a field, more precisely Z 4 p SG = d x −g R[gµν] ; where R measures the curvature of space-time • In more detail: gµν = ηµν + hµν • Now, with hµν playing the role of Aµ, we find Z 4 ρ µν SG = d x (@ρhµν)(@ h ) + ··· • Waves of hµν correspond to gravitons, just like waves of Aµ correspond to photons • Now, replace SQED with SStandard Model (that's just a minor complication....) and write S = SG + SSM : This could be our `Theory of Everything', but there are divergences .... • Divergences are a hard but solvable problem for QFT • However, these very same divergences make it very difficult to even define quantum gravity at E ∼ MPlanck String theory: `to know is to love' • String theory solves this problem in 10 dimensions: • The divergences at ~k ! 1 are now removed (cf. Timo Weigand's recent colloquium talk) • Thus, in 10 dimensions but at low energy (E 1=lstring ), we get an (essentially) unique 10d QFT: µνρ µνρ L = R[gµν] + FµνρF + HµνρH + ··· `Kaluza-Klein Compactification’ to 4 dimensions • To get the idea, let us first imagine we had a 2d theory, but need a 1d theory • We can simply consider space to have the form of a cylinder or `the surface of a rope': Image by S.
    [Show full text]
  • Lectures on Naturalness, String Landscape and Multiverse
    Lectures on Naturalness, String Landscape and Multiverse Arthur Hebecker Institute for Theoretical Physics, Heidelberg University, Philosophenweg 19, D-69120 Heidelberg, Germany 24 August, 2020 Abstract The cosmological constant and electroweak hierarchy problem have been a great inspira- tion for research. Nevertheless, the resolution of these two naturalness problems remains mysterious from the perspective of a low-energy effective field theorist. The string theory landscape and a possible string-based multiverse offer partial answers, but they are also controversial for both technical and conceptual reasons. The present lecture notes, suitable for a one-semester course or for self-study, attempt to provide a technical introduction to these subjects. They are aimed at graduate students and researchers with a solid back- ground in quantum field theory and general relativity who would like to understand the string landscape and its relation to hierarchy problems and naturalness at a reasonably technical level. Necessary basics of string theory are introduced as part of the course. This text will also benefit graduate students who are in the process of studying string theory arXiv:2008.10625v3 [hep-th] 27 Jul 2021 at a deeper level. In this case, the present notes may serve as additional reading beyond a formal string theory course. Preface This course intends to give a concise but technical introduction to `Physics Beyond the Standard Model' and early cosmology as seen from the perspective of string theory. Basics of string theory will be taught as part of the course. As a central physics theme, the two hierarchy problems (of the cosmological constant and of the electroweak scale) will be discussed in view of ideas like supersymmetry, string theory landscape, eternal inflation and multiverse.
    [Show full text]
  • Introduction to String Theory A.N
    Introduction to String Theory A.N. Schellekens Based on lectures given at the Radboud Universiteit, Nijmegen Last update 6 July 2016 [Word cloud by www.worldle.net] Contents 1 Current Problems in Particle Physics7 1.1 Problems of Quantum Gravity.........................9 1.2 String Diagrams................................. 11 2 Bosonic String Action 15 2.1 The Relativistic Point Particle......................... 15 2.2 The Nambu-Goto action............................ 16 2.3 The Free Boson Action............................. 16 2.4 World sheet versus Space-time......................... 18 2.5 Symmetries................................... 19 2.6 Conformal Gauge................................ 20 2.7 The Equations of Motion............................ 21 2.8 Conformal Invariance.............................. 22 3 String Spectra 24 3.1 Mode Expansion................................ 24 3.1.1 Closed Strings.............................. 24 3.1.2 Open String Boundary Conditions................... 25 3.1.3 Open String Mode Expansion..................... 26 3.1.4 Open versus Closed........................... 26 3.2 Quantization.................................. 26 3.3 Negative Norm States............................. 27 3.4 Constraints................................... 28 3.5 Mode Expansion of the Constraints...................... 28 3.6 The Virasoro Constraints............................ 29 3.7 Operator Ordering............................... 30 3.8 Commutators of Constraints.......................... 31 3.9 Computation of the Central Charge.....................
    [Show full text]
  • The Romance Between Maths and Physics
    The Romance Between Maths and Physics Miranda C. N. Cheng University of Amsterdam Very happy to be back in NTU indeed! Question 1: Why is Nature predictable at all (to some extent)? Question 2: Why are the predictions in the form of mathematics? the unreasonable effectiveness of mathematics in natural sciences. Eugene Wigner (1960) First we resorted to gods and spirits to explain the world , and then there were ….. mathematicians?! Physicists or Mathematicians? Until the 19th century, the relation between physical sciences and mathematics is so close that there was hardly any distinction made between “physicists” and “mathematicians”. Even after the specialisation starts to be made, the two maintain an extremely close relation and cannot live without one another. Some of the love declarations … Dirac (1938) If you want to be a physicist, you must do three things— first, study mathematics, second, study more mathematics, and third, do the same. Sommerfeld (1934) Our experience up to date justifies us in feeling sure that in Nature is actualized the ideal of mathematical simplicity. It is my conviction that pure mathematical construction enables us to discover the concepts and the laws connecting them, which gives us the key to understanding nature… In a certain sense, therefore, I hold it true that pure thought can grasp reality, as the ancients dreamed. Einstein (1934) Indeed, the most irresistible reductionistic charm of physics, could not have been possible without mathematics … Love or Hate? It’s Complicated… In the era when Physics seemed invincible (think about the standard model), they thought they didn’t need each other anymore.
    [Show full text]
  • Life at the Interface of Particle Physics and String Theory∗
    NIKHEF/2013-010 Life at the Interface of Particle Physics and String Theory∗ A N Schellekens Nikhef, 1098XG Amsterdam (The Netherlands) IMAPP, 6500 GL Nijmegen (The Netherlands) IFF-CSIC, 28006 Madrid (Spain) If the results of the first LHC run are not betraying us, many decades of particle physics are culminating in a complete and consistent theory for all non-gravitational physics: the Standard Model. But despite this monumental achievement there is a clear sense of disappointment: many questions remain unanswered. Remarkably, most unanswered questions could just be environmental, and disturbingly (to some) the existence of life may depend on that environment. Meanwhile there has been increasing evidence that the seemingly ideal candidate for answering these questions, String Theory, gives an answer few people initially expected: a huge \landscape" of possibilities, that can be realized in a multiverse and populated by eternal inflation. At the interface of \bottom- up" and \top-down" physics, a discussion of anthropic arguments becomes unavoidable. We review developments in this area, focusing especially on the last decade. CONTENTS 6. Free Field Theory Constructions 35 7. Early attempts at vacuum counting. 36 I. Introduction2 8. Meromorphic CFTs. 36 9. Gepner Models. 37 II. The Standard Model5 10. New Directions in Heterotic strings 38 11. Orientifolds and Intersecting Branes 39 III. Anthropic Landscapes 10 12. Decoupling Limits 41 A. What Can Be Varied? 11 G. Non-supersymmetric strings 42 B. The Anthropocentric Trap 12 H. The String Theory Landscape 42 1. Humans are irrelevant 12 1. Existence of de Sitter Vacua 43 2. Overdesign and Exaggerated Claims 12 2.
    [Show full text]
  • Bachas: Massive Ads Gravity from String Theory
    Massive AdS Gravity from String Theory Costas BACHAS (ENS, Paris) Conference on "Geometry and Strings’’ Schloss Ringberg, July 23 - 27, 2018 Based on two papers with Ioannis Lavdas arXiv: 1807.00591 arXiv: 1711.11372 Earlier work with John Estes arXiv: 1103.2800 If I have time, I may also comment briefly on arXiv: 1711.06722 with Bianchi & Hanany Plan of Talk 1. Foreword 2. g-Mass from holography 3. Representation merging 4. Review of N=4 AdS4/CFT3 5. g-Mass operator 6. `Scottish Bagpipes’ 7. 3 rewritings & bigravity 8. Final remarks 1 Foreword An old question: Can gravity be `higgsed’ (become massive) ? Extensive (recent & less recent) literature: Pauli, Fierz, Proc.Roy.Soc. 1939 . Nice reviews: Hinterblicher 1105.3735; de Rham 1401.4173 Schmidt-May & von Strauss 1512.00021 The question is obviously interesting, since any sound IR modification of General Relativity could have consequences for cosmology [degravitating dark energy? `mimicking dark matter’ ? . ] The main messages of this talk : — Massive AdS Gravity is part of the string-theory landscape — A quasi-universal, quantized formula for the mass Setting is 10d IIB sugra, and holographic dual CFTs If <latexit sha1_base64="RY3Mceo40A2JogR2P79cFMHL7hM=">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</latexit>
    [Show full text]
  • Tensor Modes on the String Theory Landscape Arxiv:1206.4034V1 [Hep
    Tensor modes on the string theory landscape Alexander Westphal Deutsches Elektronen-Synchrotron DESY, Theory Group, D-22603 Hamburg, Germany We attempt an estimate for the distribution of the tensor mode fraction r over the landscape of vacua in string theory. The dynamics of eternal inflation and quantum tunneling lead to a kind of democracy on the landscape, providing no bias towards large-field or small-field inflation regardless of the class of measure. The tensor mode fraction then follows the number frequency distributions of inflationary mechanisms of string theory over the landscape. We show that an estimate of the relative number frequencies for small-field vs large-field inflation, while unattainable on the whole landscape, may be within reach as a regional answer for warped Calabi-Yau flux compactifications of type IIB string theory. arXiv:1206.4034v1 [hep-th] 18 Jun 2012 June 19, 2012 Contents 1 Introduction and Motivation 2 2 Assumptions 5 2.1 Need for symmetry . 5 2.2 Properties of scalar fields in compactified string theory . 7 2.3 Populating vacua { tunneling and quantum diffusion . 8 3 An almost argument { field displacement is expensive 11 4 Counting ... 24 4.1 Eternity . 24 4.2 Democracy { tumbling down the rabbit hole . 26 4.3 Vacuum energy distribution . 31 4.4 Multitude . 32 4.5 An accessible sector of landscape . 36 5 Discussion 38 A Suppression of uphill tunneling 41 A.1 CdL tunneling in the thin-wall approximation . 41 A.2 CdL tunneling away from the thin-wall approximation . 42 A.3 Hawking-Moss tunneling - the 'no-wall' limit .
    [Show full text]
  • The String Landscape, the Swampland and The
    The String Landscape The Swampland And Our Universe Cumrun Vafa Harvard University Feb. 28, 2020 KITP, Santa Barbara https://www.cumrunvafa.orG Quantum Field Theories—without gravity included— are well understood. They beautifully describe the interaction of all the elementary particles we know. To include gravity, `Couple the QFT to Gravity’ we need to consider fluctuating metric for spacetime instead of fixed Minkowski space. However, when one tries to add gravity into the mix (in the form of gravitons) the formalism breaks down. The computation of physical processes leads to incurable infinities! This naively suggests: Quantum Field Theories cannot be coupled to gravity! This cannot be true! After all we live in a universe with both gravity and with quantum fields! Resolution? String Theory: A consistent framework which unifies quantum theory and Einstein's theory of gravity—a highly non-trivial accomplishment! Leads to consistent coupling of QFT’s to gravity. Joining and splitting of strings leads to interaction between strings Resolves the inconsistency between quantum theory and gravity Extra Dimensions One of the novel features of string theory is the prediction that there are extra dimensions, beyond 3 spatial dimensions and 1 time. These must be tiny to avoid experimental detection to date. Extra dimensions of string theory can have a large number of distinct possibilities The physical properties observed in 3+1 dimensions depends on the choice of the compact tiny space: Number of forces, particles and their masses, etc. Since there are a vast number of allowed tiny spaces which are allowed we get a huge number of consistent possible effective 3+1 dimensional theories; The String Landscape Each choice of compactification space leads to a distinct observable physics in 4 dimensions.
    [Show full text]
  • What If String Theory Has No De Sitter Vacua? Arxiv:1804.01120V2 [Hep-Th] 17 Apr 2018
    UUITP-09/18 What if string theory has no de Sitter vacua? Ulf H. Danielssona and Thomas Van Rietb b Institutionen f¨orfysik och astronomi, Uppsala Universitet, Uppsala, Sweden ulf.danielsson @ physics.uu.se cInstituut voor Theoretische Fysica, K.U. Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium thomas.vanriet @ fys.kuleuven.be Abstract We present a brief overview of attempts to construct de Sitter vacua in string theory and explain how the results of this 20-year endeavor could point to the fact that string theory harbours no de Sitter vacua at all. Making such a statement is often considered controversial and \bad news for string theory". We discuss how perhaps the opposite can be true. arXiv:1804.01120v2 [hep-th] 17 Apr 2018 Contents 1 Introduction 3 2 dS constructions in string sofar 5 2.1 Conceptual framework . .5 2.2 Classification scheme . .7 2.3 Classical . .8 2.4 Non-geometric . 10 2.5 Quantum . 11 2.5.1 IIB string theory . 12 2.5.2 Other string theories . 16 3 They all have problems? 17 3.1 Classical . 17 3.2 Non-geometric . 19 3.3 Quantum . 20 3.3.1 Anti-brane backreaction inside extra dimensions . 21 3.3.2 Anti-brane backreaction on the moduli . 23 3.3.3 Issues with non-SUSY GKP solutions? . 25 4 What now? 26 4.1 What about dark energy? . 27 4.2 What about the AdS landscape? . 27 4.3 What about dS/CFT? . 29 5 Conclusion 30 2 1 Introduction Since the middle of the 1970s string theory has been argued to be the way in which quantum mechanics and general relativity are to be unified into a theory of quantum gravity.
    [Show full text]
  • Plenary Talk at SUSY 2006
    The Landscape, Supersymmetry and Naturalness Michael Dine SUSY 2006 UC Irvine, June, 2006 The LHC: Will it Find Anything? It will almost surely find a Higgs particle. But we all hope for more. These hopes are based on the notion of naturalness. Puzzles: Cosmological constant • M /Mp • higgs θ • qcd Fermion mass hierarchy • ... • 1 Recently, in light of the landscape, naturalness has been declared (almost) dead by Douglas Susskind, Arkani- Hamed, Dimopoulos and others. Claims today: 1. The landscape actually makes the question of nat- uralness sharp. Low energy effective theories se- lected from distributions. Observed couplings, scales, may be much more common in some regions of the landscape than in others. 2. It is questions of naturalness which one has best hope to address in landscape context. Precisely questions of what is generic, of correlations, statis- tics, as opposed to hunting for particulars. 3. If you are an advocate of naturalness, the landscape [right or wrong, anthropic or not] is currently the best (theoretical) framework in which to test your ideas. (supersymmetry, warping, technicolor). 2 Aspects of Naturalness Usual notion: Quantity x naturally small if theory be- comes more symmetric in the limit that x 0. → 8π2 − Large ratios of scales from small couplings: e g2 small for g of order 1. Prior to string theory, with its original aura of unique- ness, this notion of naturalness had almost a mystical quality. As if one was worried a supreme being should not have to work to hard to make the universe more or less like it is (strongly anthropic).
    [Show full text]