SUPERGRAVITY, STRING THEORY and BLACK HOLES by Nikolay P. Bobev a Dissertation Presented to the FACULTY of the USC GRADUATE SCHO
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Band Spectrum Is D-Brane
Prog. Theor. Exp. Phys. 2016, 013B04 (26 pages) DOI: 10.1093/ptep/ptv181 Band spectrum is D-brane Koji Hashimoto1,∗ and Taro Kimura2,∗ 1Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan 2Department of Physics, Keio University, Kanagawa 223-8521, Japan ∗E-mail: [email protected], [email protected] Received October 19, 2015; Revised November 13, 2015; Accepted November 29, 2015; Published January 24 , 2016 Downloaded from ............................................................................... We show that band spectrum of topological insulators can be identified as the shape of D-branes in string theory. The identification is based on a relation between the Berry connection associated with the band structure and the Atiyah–Drinfeld–Hitchin–Manin/Nahm construction of solitons http://ptep.oxfordjournals.org/ whose geometric realization is available with D-branes. We also show that chiral and helical edge states are identified as D-branes representing a noncommutative monopole. ............................................................................... Subject Index B23, B35 1. Introduction at CERN - European Organization for Nuclear Research on July 8, 2016 Topological insulators and superconductors are one of the most interesting materials in which theo- retical and experimental progress have been intertwined each other. In particular, the classification of topological phases [1,2] provided concrete and rigorous argument on stability and the possibility of topological insulators and superconductors. The key to finding the topological materials is their electron band structure. The existence of gapless edge states appearing at spatial boundaries of the material signals the topological property. Identification of possible electron band structures is directly related to the topological nature of topological insulators. It is important, among many possible appli- cations of topological insulators, to gain insight into what kind of electron band structure is possible for topological insulators with fixed topological charges. -
Introductory Lectures on Quantum Field Theory
Introductory Lectures on Quantum Field Theory a b L. Álvarez-Gaumé ∗ and M.A. Vázquez-Mozo † a CERN, Geneva, Switzerland b Universidad de Salamanca, Salamanca, Spain Abstract In these lectures we present a few topics in quantum field theory in detail. Some of them are conceptual and some more practical. They have been se- lected because they appear frequently in current applications to particle physics and string theory. 1 Introduction These notes are based on lectures delivered by L.A.-G. at the 3rd CERN–Latin-American School of High- Energy Physics, Malargüe, Argentina, 27 February–12 March 2005, at the 5th CERN–Latin-American School of High-Energy Physics, Medellín, Colombia, 15–28 March 2009, and at the 6th CERN–Latin- American School of High-Energy Physics, Natal, Brazil, 23 March–5 April 2011. The audience on all three occasions was composed to a large extent of students in experimental high-energy physics with an important minority of theorists. In nearly ten hours it is quite difficult to give a reasonable introduction to a subject as vast as quantum field theory. For this reason the lectures were intended to provide a review of those parts of the subject to be used later by other lecturers. Although a cursory acquaintance with the subject of quantum field theory is helpful, the only requirement to follow the lectures is a working knowledge of quantum mechanics and special relativity. The guiding principle in choosing the topics presented (apart from serving as introductions to later courses) was to present some basic aspects of the theory that present conceptual subtleties. -
Duality and Strings Dieter Lüst, LMU and MPI München
Duality and Strings Dieter Lüst, LMU and MPI München Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Duality of 4 - dimensional string constructions: • Covariant lattices ⇔ (a)symmetric orbifolds (1986/87: W. Lerche, D.L., A. Schellekens ⇔ L. Ibanez, H.P. Nilles, F. Quevedo) • Intersecting D-brane models ☞ SM (?) (2000/01: R. Blumenhagen, B. Körs, L. Görlich, D.L., T. Ott ⇔ G. Aldazabal, S. Franco, L. Ibanez, F. Marchesano, R. Rabadan, A. Uranga) Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Duality of 4 - dimensional string constructions: • Covariant lattices ⇔ (a)symmetric orbifolds (1986/87: W. Lerche, D.L., A. Schellekens ⇔ L. Ibanez, H.P. Nilles, F. Quevedo) • Intersecting D-brane models ☞ SM (?) (2000/01: R. Blumenhagen, B. Körs, L. Görlich, D.L., T. Ott ⇔ G. Aldazabal, S. Franco, L. Ibanez, F. Marchesano, R. Rabadan, A. Uranga) ➢ Madrid (Spanish) Quiver ! Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. -
Arxiv:Hep-Th/0006117V1 16 Jun 2000 Oadmarolf Donald VERSION HYPER - Style
Preprint typeset in JHEP style. - HYPER VERSION SUGP-00/6-1 hep-th/0006117 Chern-Simons terms and the Three Notions of Charge Donald Marolf Physics Department, Syracuse University, Syracuse, New York 13244 Abstract: In theories with Chern-Simons terms or modified Bianchi identities, it is useful to define three notions of either electric or magnetic charge associated with a given gauge field. A language for discussing these charges is introduced and the proper- ties of each charge are described. ‘Brane source charge’ is gauge invariant and localized but not conserved or quantized, ‘Maxwell charge’ is gauge invariant and conserved but not localized or quantized, while ‘Page charge’ conserved, localized, and quantized but not gauge invariant. This provides a further perspective on the issue of charge quanti- zation recently raised by Bachas, Douglas, and Schweigert. For the Proceedings of the E.S. Fradkin Memorial Conference. Keywords: Supergravity, p–branes, D-branes. arXiv:hep-th/0006117v1 16 Jun 2000 Contents 1. Introduction 1 2. Brane Source Charge and Brane-ending effects 3 3. Maxwell Charge and Asymptotic Conditions 6 4. Page Charge and Kaluza-Klein reduction 7 5. Discussion 9 1. Introduction One of the intriguing properties of supergravity theories is the presence of Abelian Chern-Simons terms and their duals, the modified Bianchi identities, in the dynamics of the gauge fields. Such cases have the unusual feature that the equations of motion for the gauge field are non-linear in the gauge fields even though the associated gauge groups are Abelian. For example, massless type IIA supergravity contains a relation of the form dF˜4 + F2 H3 =0, (1.1) ∧ where F˜4, F2,H3 are gauge invariant field strengths of rank 4, 2, 3 respectively. -
Two-Dimensional Instantons with Bosonization and Physics of Adjoint QCD2
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Preprint ITEP–TH–21/96 Two-Dimensional Instantons with Bosonization and Physics of Adjoint QCD2. A.V. Smilga ITEP, B. Cheremushkinskaya 25, Moscow 117259, Russia Abstract We evaluate partition functions ZI in topologically nontrivial (instanton) gauge sectors in the bosonized version of the Schwinger model and in a gauged WZNW model corresponding to QCD2 with adjoint fermions. We show that the bosonized model is equivalent to the fermion model only if a particular form of the WZNW action with gauge-invariant integrand is chosen. For the exact correspondence, it is necessary to 2 integrate over the ways the gauge group SU(N)/ZN is embedded into the full O(N −1) group for the bosonized matter field. For even N, one should also take into account the 2 n contributions of both disconnected components in O(N − 1). In that case, ZI ∝ m 0 for small fermion masses where 2n0 coincides with the number of fermion zero modes in n a particular instanton background. The Taylor expansion of ZI /m 0 in mass involves only even powers of m as it should. The physics of adjoint QCD2 is discussed. We argue that, for odd N, the discrete chiral symmetry Z2 ⊗Z2 present in the action is broken spontaneously down to Z2 and the fermion condensate < λλ¯ >0 is formed. The system undergoes a first order phase transition at Tc = 0 so that the condensate is zero at an arbitrary small temperature. -
From Vibrating Strings to a Unified Theory of All Interactions
Barton Zwiebach From Vibrating Strings to a Unified Theory of All Interactions or the last twenty years, physicists have investigated F String Theory rather vigorously. The theory has revealed an unusual depth. As a result, despite much progress in our under- standing of its remarkable properties, basic features of the theory remain a mystery. This extended period of activity is, in fact, the second period of activity in string theory. When it was first discov- ered in the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics— a theoryof quarks and gluons—and despite their early promise, strings faded away. This time string theory is a credible candidate for a theoryof all interactions—a unified theoryof all forces and matter. The greatest complication that frustrated the search for such a unified theorywas the incompatibility between two pillars of twen- tieth century physics: Einstein’s General Theoryof Relativity and the principles of Quantum Mechanics. String theory appears to be 30 ) zwiebach mit physics annual 2004 the long-sought quantum mechani- cal 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. Nevertheless, intense work has demonstrated that string theory incorporates many features of the physical universe. It is reasonable to be very optimistic about the prospects of string theory. Perhaps one of the most impressive features of string theory is the appearance of gravity as one of the fluctuation modes of a closed string. Although it was not discov- ered exactly in this way, we can describe a logical path that leads to the discovery of gravity in string theory. -
Introduction to Conformal Field Theory and String
SLAC-PUB-5149 December 1989 m INTRODUCTION TO CONFORMAL FIELD THEORY AND STRING THEORY* Lance J. Dixon Stanford Linear Accelerator Center Stanford University Stanford, CA 94309 ABSTRACT I give an elementary introduction to conformal field theory and its applications to string theory. I. INTRODUCTION: These lectures are meant to provide a brief introduction to conformal field -theory (CFT) and string theory for those with no prior exposure to the subjects. There are many excellent reviews already available (or almost available), and most of these go in to much more detail than I will be able to here. Those reviews con- centrating on the CFT side of the subject include refs. 1,2,3,4; those emphasizing string theory include refs. 5,6,7,8,9,10,11,12,13 I will start with a little pre-history of string theory to help motivate the sub- ject. In the 1960’s it was noticed that certain properties of the hadronic spectrum - squared masses for resonances that rose linearly with the angular momentum - resembled the excitations of a massless, relativistic string.14 Such a string is char- *Work supported in by the Department of Energy, contract DE-AC03-76SF00515. Lectures presented at the Theoretical Advanced Study Institute In Elementary Particle Physics, Boulder, Colorado, June 4-30,1989 acterized by just one energy (or length) scale,* namely the square root of the string tension T, which is the energy per unit length of a static, stretched string. For strings to describe the strong interactions fi should be of order 1 GeV. Although strings provided a qualitative understanding of much hadronic physics (and are still useful today for describing hadronic spectra 15 and fragmentation16), some features were hard to reconcile. -
Five-Branes in Heterotic Brane-World Theories
SUSX-TH/01-037 HUB-EP-01/34 hep-th/0109173 Five-Branes in Heterotic Brane-World Theories Matthias Br¨andle1∗ and Andr´eLukas2§ 1Institut f¨ur Physik, Humboldt Universit¨at Invalidenstraße 110, 10115 Berlin, Germany 2Centre for Theoretical Physics, University of Sussex Falmer, Brighton BN1 9QJ, UK Abstract The effective action for five-dimensional heterotic M-theory in the presence of five-branes is systemat- ically derived from Hoˇrava-Witten theory coupled to an M5-brane world-volume theory. This leads to a 1 five-dimensional N = 1 gauged supergravity theory on S /Z2 coupled to four-dimensional N = 1 theories residing on the two orbifold fixed planes and an additional bulk three-brane. We analyse the properties of this action, particularly the four-dimensional effective theory associated with the domain-wall vacuum state. arXiv:hep-th/0109173v2 8 Oct 2001 The moduli K¨ahler potential and the gauge-kinetic functions are determined along with the explicit relations between four-dimensional superfields and five-dimensional component fields. ∗email: [email protected] §email: [email protected] 1 Introduction A large class of attractive five-dimensional brane-world models can be constructed by reducing Hoˇrava-Witten theory [1, 2, 3] on Calabi-Yau three-folds. This procedure has been first carried out in Ref. [4, 5, 6] and it leads 1 to gauged five-dimensional N = 1 supergravity on the orbifold S /Z2 coupled to N = 1 gauge and gauge matter multiplets located on the two four-dimensional orbifold fixed planes. It has been shown [7]–[13] that a phenomeno- logically interesting particle spectrum on the orbifold planes can be obtained by appropriate compactifications. -
Flux Tubes, Domain Walls and Orientifold Planar Equivalence
Flux tubes, domain walls and orientifold planar equivalence Agostino Patella CERN GGI, 5 May 2011 Agostino Patella (CERN) Tubes and walls GGI, 5/5/11 1 / 19 Introduction Orientifold planar equivalence Orientifold planar equivalence OrQCD 2 SU(N) gauge theory (λ = g N fixed) with Nf Dirac fermions in the antisymmetric representation is equivalent in the large-N limit and in a common sector to AdQCD 2 SU(N) gauge theory (λ = g N fixed) with Nf Majorana fermions in the adjoint representation if and only if C-symmetry is not spontaneously broken. Agostino Patella (CERN) Tubes and walls GGI, 5/5/11 2 / 19 2 Z Z ff e−N W(J) = DADψDψ¯ exp −S(A, ψ, ψ¯) + N2 J(x)O(x)d4x Introduction Orientifold planar equivalence Gauge-invariant common sector AdQCD BOSONIC C-EVEN FERMIONIC C-EVEN BOSONIC C-ODD FERMIONIC C-ODD ~ w OrQCD BOSONIC C-EVEN BOSONIC C-ODD COMMON SECTOR Agostino Patella (CERN) Tubes and walls GGI, 5/5/11 3 / 19 Introduction Orientifold planar equivalence Gauge-invariant common sector AdQCD BOSONIC C-EVEN FERMIONIC C-EVEN BOSONIC C-ODD FERMIONIC C-ODD ~ w OrQCD BOSONIC C-EVEN BOSONIC C-ODD COMMON SECTOR 2 Z Z ff e−N W(J) = DADψDψ¯ exp −S(A, ψ, ψ¯) + N2 J(x)O(x)d4x lim WOr(J) = lim WAd(J) N→∞ N→∞ Agostino Patella (CERN) Tubes and walls GGI, 5/5/11 3 / 19 Introduction Orientifold planar equivalence Gauge-invariant common sector AdQCD BOSONIC C-EVEN FERMIONIC C-EVEN BOSONIC C-ODD FERMIONIC C-ODD ~ w OrQCD BOSONIC C-EVEN BOSONIC C-ODD COMMON SECTOR 2 Z Z ff e−N W(J) = DADψDψ¯ exp −S(A, ψ, ψ¯) + N2 J(x)O(x)d4x hO(x ) ··· O(xn)i hO(x ) ··· -
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..................... -
Dirac Equation for Strings in Minkowski Space-Time and Then Study the Radial Vibrations of the String
Dirac equation for strings Maciej Trzetrzelewski ∗ M. Smoluchowski Institute of Physics, Jagiellonian University, Lojasiewicza, St. 11, 30-348 Krak´ow, Poland Abstract Starting with a Nambu-Goto action, a Dirac-like equation can be constructed by taking the square-root of the momentum constraint. The eigenvalues of the resulting Hamiltonian are real and correspond to masses of the excited string. In particular there are no tachyons. A special case of radial oscillations of a closed string in Minkowski space-time admits exact solutions in terms of wave functions of the harmonic oscillator. 1 Introduction In 1962 Dirac considered the possibility that leptons may be described arXiv:1302.5907v3 [hep-th] 14 Feb 2018 by extended objects of spherical topology [1, 2]. In this way one could understand the muon as an excitation of the ground state of the membrane - the electron. Anticipating Nambu [3] and Goto [4] by almost a decade he introduced what is now known as a generalization of the Nambu-Goto action to the case of membranes. Using Bohr- Sommerfeld approximation for the Hamiltonian corresponding to the radial mode, one can then show [1] that the mass of the first excitation is about 53me where me is the mass of the electron. This is about a quarter of the observed mass of the muon. In fact, when instead of ∗e-mail: [email protected] 1 the Bohr-Sommerfeld approximation one uses, more precise, numeri- cal methods one finds that the correct value of the first excitation is about 43me [5, 6]. Therefore Dirac’s model ”explains” 1/5th of the actual value of the muon mass. -
Chapter 9: the 'Emergence' of Spacetime in String Theory
Chapter 9: The `emergence' of spacetime in string theory Nick Huggett and Christian W¨uthrich∗ May 21, 2020 Contents 1 Deriving general relativity 2 2 Whence spacetime? 9 3 Whence where? 12 3.1 The worldsheet interpretation . 13 3.2 T-duality and scattering . 14 3.3 Scattering and local topology . 18 4 Whence the metric? 20 4.1 `Background independence' . 21 4.2 Is there a Minkowski background? . 24 4.3 Why split the full metric? . 27 4.4 T-duality . 29 5 Quantum field theoretic considerations 29 5.1 The graviton concept . 30 5.2 Graviton coherent states . 32 5.3 GR from QFT . 34 ∗This is a chapter of the planned monograph Out of Nowhere: The Emergence of Spacetime in Quantum Theories of Gravity, co-authored by Nick Huggett and Christian W¨uthrich and under contract with Oxford University Press. More information at www.beyondspacetime.net. The primary author of this chapter is Nick Huggett ([email protected]). This work was sup- ported financially by the ACLS and the John Templeton Foundation (the views expressed are those of the authors not necessarily those of the sponsors). We want to thank Tushar Menon and James Read for exceptionally careful comments on a draft this chapter. We are also grateful to Niels Linnemann for some helpful feedback. 1 6 Conclusions 35 This chapter builds on the results of the previous two to investigate the extent to which spacetime might be said to `emerge' in perturbative string the- ory. Our starting point is the string theoretic derivation of general relativity explained in depth in the previous chapter, and reviewed in x1 below (so that the philosophical conclusions of this chapter can be understood by those who are less concerned with formal detail, and so skip the previous one).