Instantons, Symmetries and Anomalies in Five Dimensions
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Kaluza-Klein Gravity, Concentrating on the General Rel- Ativity, Rather Than Particle Physics Side of the Subject
Kaluza-Klein Gravity J. M. Overduin Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, British Columbia, Canada, V8W 3P6 and P. S. Wesson Department of Physics, University of Waterloo, Ontario, Canada N2L 3G1 and Gravity Probe-B, Hansen Physics Laboratories, Stanford University, Stanford, California, U.S.A. 94305 Abstract We review higher-dimensional unified theories from the general relativity, rather than the particle physics side. Three distinct approaches to the subject are identi- fied and contrasted: compactified, projective and noncompactified. We discuss the cosmological and astrophysical implications of extra dimensions, and conclude that none of the three approaches can be ruled out on observational grounds at the present time. arXiv:gr-qc/9805018v1 7 May 1998 Preprint submitted to Elsevier Preprint 3 February 2008 1 Introduction Kaluza’s [1] achievement was to show that five-dimensional general relativity contains both Einstein’s four-dimensional theory of gravity and Maxwell’s the- ory of electromagnetism. He however imposed a somewhat artificial restriction (the cylinder condition) on the coordinates, essentially barring the fifth one a priori from making a direct appearance in the laws of physics. Klein’s [2] con- tribution was to make this restriction less artificial by suggesting a plausible physical basis for it in compactification of the fifth dimension. This idea was enthusiastically received by unified-field theorists, and when the time came to include the strong and weak forces by extending Kaluza’s mechanism to higher dimensions, it was assumed that these too would be compact. This line of thinking has led through eleven-dimensional supergravity theories in the 1980s to the current favorite contenders for a possible “theory of everything,” ten-dimensional superstrings. -
D-Instanton Perturbation Theory
D-instanton Perturbation Theory Ashoke Sen Harish-Chandra Research Institute, Allahabad, India Sao Paolo, June 2020 1 Plan: 1. Overview of the problem and the solution 2. Review of basic aspects of world-sheet string theory and string field theory 3. Some explicit computations A.S., arXiv:1908.02782, 2002.04043, work in progress 2 The problem 3 String theory began with Veneziano amplitude – tree level scattering amplitude of four tachyons in open string theory World-sheet expression for the amplitude (in α0 = 1 unit) Z 1 dy y2p1:p2 (1 − y)2p2:p3 0 – diverges for 2p1:p2 ≤ −1 or 2p2:p3 ≤ −1. Our convention: a:b ≡ −a0b0 + ~a:~b Conventional viewpoint: Define the amplitude for 2p1:p2 > −1, 2p2:p3 > −1 and then analytically continue to the other kinematic regions. 4 However, analytic continuation does not always work It may not be possible to move away from the singularity by changing the external momenta Examples: Mass renormalization, Vacuum shift – discussed earlier In these lectures we shall discuss another situation where analytic continuation fails – D-instanton contribution to string amplitudes 5 D-instanton: A D-brane with Dirichlet boundary condition on all non-compact directions including (euclidean) time. D-instantons give non-perturbative contribution to string amplitudes that are important in many situations Example: KKLT moduli stabilization uses non-perturbative contribution from D-instanton (euclidean D3-brane) Systematic computation of string amplitudes in such backgrounds will require us to compute amplitudes in the presence of D-instantons Problem: Open strings living on the D-instanton do not carry any continuous momenta ) we cannot move away from the singularities by varying the external momenta 6 Some examples: Let X be the (euclidean) time direction Since the D-instanton is localized at some given euclidean time, it has a zero mode that translates it along time direction 4-point function of these zero modes: Z 1 A = dy y−2 + (y − 1)−2 + 1 0 Derivation of this expression will be discussed later. -
Holography Principle and Topology Change in String Theory 1 Abstract
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server SNUTP 98-089 hep-th/9807241 Holography Principle and Topology Change in String Theory 1 Soo-Jong Rey Physics Department, Seoul National University, Seoul 151-742 KOREA abstract D-instantons of Type IIB string theory are Ramond-Ramond counterpart of Giddings-Strominger wormholes connecting two asymptotic regions of spacetime. Such wormholes, according to Coleman, might lead to spacetime topology change, third-quantized baby universes and prob- abilistic determination of fundamental coupling parameters. Utilizing correspondence between AdS5 × M5 Type IIB supergravity and d = 4 super Yang-Mills theory, we point out that topol- ogy change and sum over topologies not only take place in string theory but also are required for consistency with holography. Nevertheless, we argue that the effects of D-instanton wormholes remain completely deterministic, in sharp contrast to Coleman’s scenario. 1Work supported in part by KOSEF SRC-Program, Ministry of Education Grant BSRI 98-2418, SNU Re- search Fund and Korea Foundation for Advanced Studies Faculty Fellowship. One of the most vexing problems in quantum gravity has been the issue of spacetime topol- ogy change: whether topology of spacetime can fluctuate and, if so, spacetime of different topologies should be summed over. Any positive answer to this question would bear profound implications to the fundamental interactions of Nature. For example, in Coleman’s scenario [1] of baby universes [2], fluctuation of spacetime topology induce effective lon-local interactions and third quantization of the universe thereof 2. As a result, the cosmological constant is no longer a calculable, deterministic parameter but is turned into a quantity of probabilistic dis- tribution sharply peaked around zero. -
Spontaneous Breaking of Conformal Invariance and Trace Anomaly
Spontaneous Breaking of Conformal Invariance and Trace Anomaly Matching ∗ A. Schwimmera and S. Theisenb a Department of Physics of Complex Systems, Weizmann Institute, Rehovot 76100, Israel b Max-Planck-Institut f¨ur Gravitationsphysik, Albert-Einstein-Institut, 14476 Golm, Germany Abstract We argue that when conformal symmetry is spontaneously broken the trace anomalies in the broken and unbroken phases are matched. This puts strong constraints on the various couplings of the dilaton. Using the uniqueness of the effective action for the Goldstone supermultiplet for broken = 1 supercon- formal symmetry the dilaton effective action is calculated. N arXiv:1011.0696v1 [hep-th] 2 Nov 2010 November 2010 ∗ Partially supported by GIF, the German-Israeli Foundation for Scientific Research, the Minerva Foundation, DIP, the German-Israeli Project Cooperation and the Einstein Center of Weizmann Institute. 1. Introduction The matching of chiral anomalies of the ultraviolet and infrared theories related by a massive flow plays an important role in understanding the dynamics of these theories. In particular using the anomaly matching the spontaneous breaking of chiral symmetry in QCD like theories was proven [1]. For supersymmetric gauge theories chiral anomaly matching provides constraints when different theories are related by “non abelian” duality in the infrared NS. The matching involves the equality of a finite number of parameters, “the anomaly coefficients” defined as the values of certain Green’s function at a very special singular point in phase space. The Green’s function themselves have very different structure at the two ends of the flow. The massive flows relate by definition conformal theories in the ultraviolet and infrared but the trace anomalies of the two theories are not matched: rather the flow has the property that the a-trace anomaly coefficient decreases along it [2]. -
Gravity, Scale Invariance and the Hierarchy Problem
Motivation Setup Warm-up: Dilaton+Gravity One example: Higgs+Gravity Further Examples: Higgs+Dilaton+Gravity Discussion and Outlook Backups Gravity, Scale Invariance and the Hierarchy Problem M. Shaposhnikov, A. Shkerin EPFL & INR RAS Based on arXiv:1803.08907, arXiv:1804.06376 QUARKS-2018 Valday, May 31, 2018 1 / 39 Motivation Setup Warm-up: Dilaton+Gravity One example: Higgs+Gravity Further Examples: Higgs+Dilaton+Gravity Discussion and Outlook Backups Overview 1 Motivation 2 Setup 3 Warm-up: Dilaton+Gravity 4 One example: Higgs+Gravity 5 Further Examples: Higgs+Dilaton+Gravity 6 Discussion and Outlook 2 / 39 Motivation Setup Warm-up: Dilaton+Gravity One example: Higgs+Gravity Further Examples: Higgs+Dilaton+Gravity Discussion and Outlook Backups Drowning by numbers The fact is that G 2 F ~ ∼ 1033, where G | Fermi constant, G | Newton constant 2 F N GN c Two aspects of the hierarchy problem (G. F. Giudice'08): \classical" \quantum": Let MX be some heavy mass scale. Then one expects 2 2 δmH;X ∼ MX : Even if one assumes that there are no heavy thresholds beyond the EW scale, then, naively, 2 2 δmH;grav: ∼ MP : 3 / 39 Motivation Setup Warm-up: Dilaton+Gravity One example: Higgs+Gravity Further Examples: Higgs+Dilaton+Gravity Discussion and Outlook Backups EFT approach and beyond A common approach to the hierarchy problem lies within the effective field theory framework: Low energy description of Nature, provided by the SM, can be affected by an unknown UV physics only though a finite set of parameters This \naturalness principle" is questioned now in light of the absence of signatures of new physics at the TeV scale. -
Mixed Anomalies of Chiral Algebras Compactified to Smooth Quasi
MIXED ANOMALIES OF CHIRAL ALGEBRAS COMPACTIFIED TO SMOOTH QUASI-PROJECTIVE SURFACES MAKOTO SAKURAI Abstract. Some time ago, the chiral algebra theory of Beilinson- Drinfeld[BD] was expected to play a central role in the conver- gence of divergence in mathematical physics of superstring theory for quantization of gauge theory and gravity. Naively, this al- gebra plays an important role in a holomorphic conformal field theory with a non-negative integer graded conformal dimension, whose target space does not necessarily have the vanishing first Chern class. This algebra has two definitions until now: one is that by Malikov-Schechtman-Vaintrob by gluing affine patches, and the other is that of Kapranov-Vasserot by gluing the formal loop spaces. I will use the new definition of Nekrasov by simplifying Malikov-Schechtman-Vaintrob in order to compute the obstruction classes of gerbes of chiral differential operators. In this paper, I will examine the two independent Ans¨atze (or working hypotheses) of Witten’s = (0, 2) heterotic strings and Nekrasov’s generalized complex geometry,N after Hitchin and Gualtieri, are consistent in the case of CP2, which has 3 affine patches and is expected to have the “first Pontryagin anomaly”. I also scrutinized the physical meanings of 2 dimensional toric Fano manifolds, or rather toric del Pezzo surfaces, obtained by blowing up the non-colinear 1, 2, 3 points of CP2. The obstruction classes of gerbes of them coincide with the second Chern char- acters obtained by the Riemann-Roch theorem and in particular vanishes for 1 point blowup, which means that one of the gravita- tional anomalies vanishes for a non-Calabi-Yau manifold compact- arXiv:0712.2318v5 [hep-th] 25 Feb 2015 ification. -
Supersymmetry and the Multi-Instanton Measure
View metadata, citation and similar papers at core.ac.uk brought to you by CORE hep-th/9708036provided by CERN Document Server Supersymmetry and the Multi-Instanton Measure Nicholas Dorey Physics Department, University of Wales Swansea Swansea SA2 8PP UK [email protected] Valentin V. Khoze Department of Physics, Centre for Particle Theory, University of Durham Durham DH1 3LE UK [email protected] and Michael P. Mattis Theoretical Division T-8, Los Alamos National Laboratory Los Alamos, NM 87545 USA [email protected] We propose explicit formulae for the integration measure on the moduli space of charge-n ADHM multi-instantons in N = 1 and N =2super- symmetric gauge theories. The form of this measure is fixed by its (su- per)symmetries as well as the physical requirement of clustering in the limit of large spacetime separation between instantons. We test our proposals against known expressions for n ≤ 2. Knowledge of the measure for all n al- lows us to revisit, and strengthen, earlier N = 2 results, chiefly: (1) For any number of flavors NF , we provide a closed formula for Fn, the n-instanton contribution to the Seiberg-Witten prepotential, as a finite-dimensional col- lective coordinate integral. This amounts to a solution, in quadratures, of the Seiberg-Witten models, without appeal to electric-magnetic duality. (2) In the conformal case NF =4,this means reducing to quadratures the previously unknown finite renormalization that relates the microscopic and effective coupling constants, τmicro and τeff. (3) Similar expressions are given for the 4-derivative/8-fermion term in the gradient expansion of N = 2 supersymmetric QCD. -
A Note on the Chiral Anomaly in the Ads/CFT Correspondence and 1/N 2 Correction
NEIP-99-012 hep-th/9907106 A Note on the Chiral Anomaly in the AdS/CFT Correspondence and 1=N 2 Correction Adel Bilal and Chong-Sun Chu Institute of Physics, University of Neuch^atel, CH-2000 Neuch^atel, Switzerland [email protected] [email protected] Abstract According to the AdS/CFT correspondence, the d =4, =4SU(N) SYM is dual to 5 N the Type IIB string theory compactified on AdS5 S . A mechanism was proposed previously that the chiral anomaly of the gauge theory× is accounted for to the leading order in N by the Chern-Simons action in the AdS5 SUGRA. In this paper, we consider the SUGRA string action at one loop and determine the quantum corrections to the Chern-Simons\ action. While gluon loops do not modify the coefficient of the Chern- Simons action, spinor loops shift the coefficient by an integer. We find that for finite N, the quantum corrections from the complete tower of Kaluza-Klein states reproduce exactly the desired shift N 2 N 2 1 of the Chern-Simons coefficient, suggesting that this coefficient does not receive→ corrections− from the other states of the string theory. We discuss why this is plausible. 1 Introduction According to the AdS/CFT correspondence [1, 2, 3, 4], the =4SU(N) supersymmetric 2 N gauge theory considered in the ‘t Hooft limit with λ gYMNfixed is dual to the IIB string 5 ≡ theory compactified on AdS5 S . The parameters of the two theories are identified as 2 4 × 4 gYM =gs, λ=(R=ls) and hence 1=N = gs(ls=R) . -
Report of Contributions
KEK Theory workshop 2019 Report of Contributions https://conference-indico.kek.jp/e/80 KEK Theory wor … / Report of Contributions Invited talk Contribution ID: 2 Type: not specified Invited talk October 1, 2021 Page 1 KEK Theory wor … / Report of Contributions Short talk Contribution ID: 3 Type: not specified Short talk October 1, 2021 Page 2 KEK Theory wor … / Report of Contributions Poster Contribution ID: 4 Type: not specified Poster October 1, 2021 Page 3 KEK Theory wor … / Report of Contributions Quantum Gravity and Naturalness Contribution ID: 5 Type: not specified Quantum Gravity and Naturalness Tuesday, 3 December 2019 10:30 (40 minutes) We discuss the possibility that naturalness can be understood as an effect of quantum gravity. In particular, we will consider a mechanism by which the electroweak scale is naturally obtained from the Planck scale. Presenter: Prof. KAWAI, Hikaru Session Classification: Invited talks October 1, 2021 Page 4 KEK Theory wor … / Report of Contributions Status of asymptotic safety in … Contribution ID: 6 Type: not specified Status of asymptotic safety in gravity-matter systems Tuesday, 3 December 2019 11:30 (40 minutes) Asymptotically safe quantum gravity is one of candidates for quantum gravity. It is essential that there exists a non-trivial fixed point for gravitational couplings. In this talk we review the current status of the asymptotic safety scenario for gravity-matter systems. Presenter: Dr YAMADA, Masatoshi Session Classification: Invited talks October 1, 2021 Page 5 KEK Theory wor … / Report of Contributions An Approach to Quantum Gravity … Contribution ID: 7 Type: not specified An Approach to Quantum Gravity – Asymptotic Safety – Tuesday, 3 December 2019 13:30 (40 minutes) We explain an approach to formulate quantum gravity within the framework of local quantum field theory using functional renormalization group. -
Instanton Operators in Five-Dimensional Gauge
MTH-KCL/2014-20 QMUL-PH-14-25 Instanton Operators in Five-Dimensional Gauge Theories N. Lambert a,∗, C. Papageorgakis b,† and M. Schmidt-Sommerfeld c,d,‡ aDepartment of Mathematics King’s College London, WC2R 2LS, UK bCRST and School of Physics and Astronomy Queen Mary University of London, E1 4NS, UK cArnold-Sommerfeld-Center f¨ur Theoretische Physik, LMU M¨unchen Theresienstraße 37, 80333 M¨unchen, Germany dExcellence Cluster Universe, Technische Universit¨at M¨unchen Boltzmannstraße 2, 85748 Garching, Germany Abstract We discuss instanton operators in five-dimensional Yang-Mills gauge theo- ries. These are defined as disorder operators which create a non-vanishing arXiv:1412.2789v3 [hep-th] 4 Jun 2015 second Chern class on a four-sphere surrounding their insertion point. As such they may be thought of as higher-dimensional analogues of three- dimensional monopole (or ‘t Hooft) operators. We argue that they play an important role in the enhancement of the Lorentz symmetry for maximally supersymmetric Yang-Mills to SO(1, 5) at strong coupling. ∗E-mail address: [email protected] †E-mail address: [email protected] ‡E-mail address: [email protected] 1 Introduction One of the more dramatic results to come out of the study of strongly coupled string theory and M-theory was the realisation that there exist UV-complete quantum super- conformal field theories (SCFTs) in five and six dimensions [1–5]. These theories then provide UV completions to a variety of perturbatively non-renormalisable five-dimensional (5D) Yang-Mills theories. In this paper we will consider the notion of ‘instanton operators’ (or Yang operators) and explore their role in five-dimensional Yang-Mills. -
Einstein and the Kaluza-Klein Particle
ITFA-99-28 Einstein and the Kaluza-Klein particle Jeroen van Dongen1 Institute for Theoretical Physics, University of Amsterdam Valckeniersstraat 65 1018 XE Amsterdam and Joseph Henry Laboratories, Princeton University Princeton NJ 08544 Abstract In his search for a unified field theory that could undercut quantum mechanics, Einstein considered five dimensional classical Kaluza-Klein theory. He studied this theory most intensively during the years 1938-1943. One of his primary objectives was finding a non-singular particle solution. In the full theory this search got frustrated and in the x5-independent theory Einstein, together with Pauli, argued it would be impossible to find these structures. Keywords: Einstein; Unified Field Theory; Kaluza-Klein Theory; Quantization; Soli- tons 1 Introduction After having formulated general relativity Albert Einstein did not immediately focus on the unification of electromagnetism and gravity in a classical field theory - the issue that would characterize much of his later work. It was still an open question to him whether arXiv:gr-qc/0009087v1 26 Sep 2000 relativity and electrodynamics together would cast light on the problem of the structure of matter [18]. Rather, in a 1916 paper on gravitational waves he anticipated a different development: since the electron in its atomic orbit would radiate gravitationally, something that cannot “occur in reality”, he expected quantum theory would have to change not only the ”Maxwellian electrodynamics, but also the new theory of gravitation” [19]2. Einstein’s position, however, gradually changed. From about 1919 onwards, he took a strong interest in the unification programme3. In later years, after about 1926, he hoped that he would find a particular classical unified field theory that could undercut quantum theory. -
Dark Energy and Inflation from Gravitational Waves
universe Article Dark Energy and Inflation from Gravitational Waves Leonid Marochnik Department of Physics, East-West Space Science Center, University of Maryland, College Park, MD 20742, USA; [email protected] Received: 2 July 2017; Accepted: 10 October 2017; Published: 18 October 2017 Abstract: In this seven-part paper, we show that gravitational waves (classical and quantum) produce the accelerated de Sitter expansion at the start and at the end of the cosmological evolution of the Universe. In these periods, the Universe contains no matter fields but contains classical and quantum metric fluctuations, i.e., it is filled with classical and quantum gravitational waves. In such evolution of the Universe, dominated by gravitational waves, the de Sitter state is the exact solution to the self-consistent equations for classical and quantum gravitational waves and background geometry for the empty space-time with FLRW metric. In both classical and quantum cases, this solution is of the instanton origin since it is obtained in the Euclidean space of imaginary time with the subsequent analytic continuation to real time. The cosmological acceleration from gravitational waves provides a transparent physical explanation to the coincidence, threshold and “old cosmological constant” paradoxes of dark energy avoiding recourse to the anthropic principle. The cosmological acceleration from virtual gravitons at the start of the Universe evolution produces inflation, which is consistent with the observational data on CMB anisotropy. Section 1 is devoted to cosmological acceleration from classical gravitational waves. Section 2 is devoted to the theory of virtual gravitons in the Universe. Section 3 is devoted to cosmological acceleration from virtual gravitons.