Vertex Operator Algebras, Modular Forms and Moonshine
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Flavor Moonshine
Prog. Theor. Exp. Phys. 2020, 013B03 (20 pages) DOI: 10.1093/ptep/ptz137 Flavor moonshine Shotaro Shiba Funai1,∗ Hirotaka Sugawara2,∗ 1Physics and Biology Unit, Okinawa Institute of Science and Technology (OIST), 1919-1 Tancha, Onna-son, Kunigami-gun, Okinawa 904-0495, Japan 2High Energy Accelerator Research Organization (KEK), 1-1 Oho, Tsukuba, Ibaraki 305-0801, Japan ∗E-mail: [email protected], [email protected] Received August 30, 2019; Revised October 17, 2019; Accepted October 23, 2019; Published January 13, 2020 ................................................................................................................... The flavor moonshine hypothesis is formulated to suppose that all particle masses (leptons, quarks, Higgs, and gauge particles—more precisely, their mass ratios) are expressed as coef- ficients in the Fourier expansion of some modular forms just as, in mathematics, dimensions of representations of a certain group are expressed as coefficients in the Fourier expansion of some modular forms. The mysterious hierarchical structure of the quark and lepton masses is thus attributed to that of the Fourier coefficient matrices of certain modular forms. Our inten- tion here is not to prove this hypothesis starting from some physical assumptions but rather to demonstrate that this hypothesis is experimentally verified and, assuming that the string theory correctly describes the natural law, to calculate the geometry (Kähler potential and the metric) of the moduli space of the Calabi–Yau manifold, thus providing a way to calculate the metric of the Calabi–Yau manifold itself directly from the experimental data. ................................................................................................................... Subject Index B41, B55 1. Introduction Some researchers, including one of the authors of this work (H.S.), have been working on flavor physics, assuming that some discrete symmetry plays an important role in its understanding [1–9]; S3, S4, A4, etc. -
Umbral Moonshine and K3 Surfaces Arxiv:1406.0619V3 [Hep-Th]
SLAC-PUB-16469 Umbral Moonshine and K3 Surfaces Miranda C. N. Cheng∗1 and Sarah Harrisony2 1Institute of Physics and Korteweg-de Vries Institute for Mathematics, University of Amsterdam, Amsterdam, the Netherlandsz 2Stanford Institute for Theoretical Physics, Department of Physics, and Theory Group, SLAC, Stanford University, Stanford, CA 94305, USA Abstract Recently, 23 cases of umbral moonshine, relating mock modular forms and finite groups, have been discovered in the context of the 23 even unimodular Niemeier lattices. One of the 23 cases in fact coincides with the so-called Mathieu moonshine, discovered in the context of K3 non-linear sigma models. In this paper we establish a uniform relation between all 23 cases of umbral moonshine and K3 sigma models, and thereby take a first step in placing umbral moonshine into a geometric and physical context. This is achieved by relating the ADE root systems of the Niemeier lattices to the ADE du Val singularities that a K3 surface can develop, and the configuration of smooth rational curves in their resolutions. A geometric interpretation of our results is given in terms of the marking of K3 surfaces by Niemeier lattices. arXiv:1406.0619v3 [hep-th] 18 Mar 2015 ∗[email protected] [email protected] zOn leave from CNRS, Paris. 1 This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-76SF00515 and HEP. Umbral Moonshine and K3 Surfaces 2 Contents 1 Introduction and Summary 3 2 The Elliptic Genus of Du Val Singularities 8 3 Umbral Moonshine and Niemeier Lattices 14 4 Umbral Moonshine and the (Twined) K3 Elliptic Genus 20 5 Geometric Interpretation 27 6 Discussion 30 A Special Functions 32 B Calculations and Proofs 34 C The Twining Functions 41 References 48 Umbral Moonshine and K3 Surfaces 3 1 Introduction and Summary Mock modular forms are interesting functions playing an increasingly important role in various areas of mathematics and theoretical physics. -
The Top Yukawa Coupling from 10D Supergravity with E8 × E8 Matter
hep-th/9804107 ITEP-98-11 The top Yukawa coupling from 10D supergravity with E E matter 8 × 8 K.Zyablyuk1 Institute of Theoretical and Experimental Physics, Moscow Abstract We consider the compactification of N=1, D=10 supergravity with E E Yang- 8 × 8 Mills matter to N=1, D=4 model with 3 generations. With help of embedding SU(5) → SO(10) E E we find the value of the top Yukawa coupling λ = 16πα =3 → 6 → 8 t GUT at the GUT scale. p 1 Introduction Although superstring theories have great success and today are the best candidates for a quantum theory unifying all interactions, they still do not predict any experimentally testable value, mostly because there is no unambiguous procedure of compactification of extra spatial dimensions. On the other hand, many phenomenological models based on the unification group SO(10) were constructed (for instance [1]). They describe quarks and leptons in representa- tions 161,162,163 and Higgses, responsible for SU(2) breaking, in 10. Basic assumption of these models is that there is only one Yukawa coupling 163 10 163 at the GUT scale, which gives masses of third generation. Masses of first two families· and· mixings are generated due to the interaction with additional superheavy ( MGUT ) states in 16 + 16, 45, 54. Such models explain generation mass hierarchy and allow∼ to express all Yukawa matrices, which well fit into experimentally observable pattern, in terms of few unknown parameters. Models of [1] are unlikely derivable from ”more fundamental” theory like supergrav- ity/string. Nevertheless, something similar can be constructed from D=10 supergravity coupled to E8 E8 matter, which is low-energy limit of heterotic string [2]. -
Arxiv:1805.06347V1 [Hep-Th] 16 May 2018 Sa Rte O H Rvt Eerhfudto 08Awar 2018 Foundation Research Gravity the for Written Essay Result
Maximal supergravity and the quest for finiteness 1 2 3 Sudarshan Ananth† , Lars Brink∗ and Sucheta Majumdar† † Indian Institute of Science Education and Research Pune 411008, India ∗ Department of Physics, Chalmers University of Technology S-41296 G¨oteborg, Sweden and Division of Physics and Applied Physics, School of Physical and Mathematical Sciences Nanyang Technological University, Singapore 637371 March 28, 2018 Abstract We show that N = 8 supergravity may possess an even larger symmetry than previously believed. Such an enhanced symmetry is needed to explain why this theory of gravity exhibits ultraviolet behavior reminiscent of the finite N = 4 Yang-Mills theory. We describe a series of three steps that leads us to this result. arXiv:1805.06347v1 [hep-th] 16 May 2018 Essay written for the Gravity Research Foundation 2018 Awards for Essays on Gravitation 1Corresponding author, [email protected] [email protected] [email protected] Quantum Field Theory describes three of the four fundamental forces in Nature with great precision. However, when attempts have been made to use it to describe the force of gravity, the resulting field theories, are without exception, ultraviolet divergent and non- renormalizable. One striking aspect of supersymmetry is that it greatly reduces the diver- gent nature of quantum field theories. Accordingly, supergravity theories have less severe ultraviolet divergences. Maximal supergravity in four dimensions, N = 8 supergravity [1], has the best ultraviolet properties of any field theory of gravity with two derivative couplings. Much of this can be traced back to its three symmetries: Poincar´esymmetry, maximal supersymmetry and an exceptional E7(7) symmetry. -
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..................... -
S-Duality-And-M5-Mit
N . More on = 2 S-dualities and M5-branes .. Yuji Tachikawa based on works in collaboration with L. F. Alday, B. Wecht, F. Benini, S. Benvenuti, D. Gaiotto November 2009 Yuji Tachikawa (IAS) November 2009 1 / 47 Contents 1. Introduction 2. S-dualities 3. A few words on TN 4. 4d CFT vs 2d CFT Yuji Tachikawa (IAS) November 2009 2 / 47 Montonen-Olive duality • N = 4 SU(N) SYM at coupling τ = θ=(2π) + (4πi)=g2 equivalent to the same theory coupling τ 0 = −1/τ • One way to ‘understand’ it: start from 6d N = (2; 0) theory, i.e. the theory on N M5-branes, put on a torus −1/τ τ 0 1 0 1 • Low energy physics depends only on the complex structure S-duality! Yuji Tachikawa (IAS) November 2009 3 / 47 S-dualities in N = 2 theories • You can wrap N M5-branes on a more general Riemann surface, possibly with punctures, to get N = 2 superconformal field theories • Different limits of the shape of the Riemann surface gives different weakly-coupled descriptions, giving S-dualities among them • Anticipated by [Witten,9703166], but not well-appreciated until [Gaiotto,0904.2715] Yuji Tachikawa (IAS) November 2009 4 / 47 Contents 1. Introduction 2. S-dualities 3. A few words on TN 4. 4d CFT vs 2d CFT Yuji Tachikawa (IAS) November 2009 5 / 47 Contents 1. Introduction 2. S-dualities 3. A few words on TN 4. 4d CFT vs 2d CFT Yuji Tachikawa (IAS) November 2009 6 / 47 S-duality in N = 2 . SU(2) with Nf = 4 . -
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. -
E 8 in N= 8 Supergravity in Four Dimensions
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Chalmers Research E 8 in N= 8 supergravity in four dimensions Downloaded from: https://research.chalmers.se, 2019-05-11 18:56 UTC Citation for the original published paper (version of record): Ananth, S., Brink, L., Majumdar, S. (2018) E 8 in N= 8 supergravity in four dimensions Journal of High Energy Physics, 2018(1) http://dx.doi.org/10.1007/JHEP01(2018)024 N.B. When citing this work, cite the original published paper. research.chalmers.se offers the possibility of retrieving research publications produced at Chalmers University of Technology. It covers all kind of research output: articles, dissertations, conference papers, reports etc. since 2004. research.chalmers.se is administrated and maintained by Chalmers Library (article starts on next page) Published for SISSA by Springer Received: November 30, 2017 Accepted: December 23, 2017 Published: January 8, 2018 E8 in N = 8 supergravity in four dimensions Sudarshan Ananth,a Lars Brinkb,c and Sucheta Majumdara aIndian Institute of Science Education and Research, Pune 411008, India bDepartment of Physics, Chalmers University of Technology, S-41296 G¨oteborg, Sweden cDivision of Physics and Applied Physics, School of Physical and Mathematical Sciences, Nanyang Technological University, 637371, Singapore E-mail: [email protected], [email protected], [email protected] Abstract: We argue that = 8 supergravity in four dimensions exhibits an exceptional N E8(8) symmetry, enhanced from the known E7(7) invariance. Our procedure to demonstrate this involves dimensional reduction of the = 8 theory to d = 3, a field redefinition to N render the E8(8) invariance manifest, followed by dimensional oxidation back to d = 4. -
Monstrous Entanglement JHEP10(2017)147 ] (Or Its Chiral 8 [ 3 20 6 22 11 15 4 22 28 9 16 29 26 , As Its Automorphism Group
Published for SISSA by Springer Received: September 1, 2017 Accepted: October 12, 2017 Published: October 20, 2017 Monstrous entanglement JHEP10(2017)147 Diptarka Das,a Shouvik Dattab and Sridip Pala aDepartment of Physics, University of California San Diego, 9500 Gilman Drive, La Jolla, CA 92093, U.S.A. bInstitut f¨urTheoretische Physik, Eidgen¨ossischeTechnische Hochschule Z¨urich, Wolfgang-Pauli-Strasse 27, 8049 Z¨urich,Switzerland E-mail: [email protected], [email protected], [email protected] Abstract: The Monster CFT plays an important role in moonshine and is also conjectured to be the holographic dual to pure gravity in AdS3. We investigate the entanglement and R´enyi entropies of this theory along with other extremal CFTs. The R´enyi entropies of a single interval on the torus are evaluated using the short interval expansion. Each order in the expansion contains closed form expressions in the modular parameter. The leading terms in the q-series are shown to precisely agree with the universal corrections to R´enyi entropies at low temperatures. Furthermore, these results are shown to match with bulk computations of R´enyi entropy using the one-loop partition function on handlebodies. We also explore some features of R´enyi entropies of two intervals on the plane. Keywords: Conformal Field Theory, AdS-CFT Correspondence, Field Theories in Lower Dimensions, Discrete Symmetries ArXiv ePrint: 1708.04242 Open Access, c The Authors. https://doi.org/10.1007/JHEP10(2017)147 Article funded by SCOAP3. Contents 1 Introduction1 2 Short interval expansion -
Final Report (PDF)
Novel Approaches to the Finite Simple Groups John McKay (Concordia University), Roland Friedrich (Humboldt University Berlin) 22. April–29. April 2012 1 Motivation It is now accepted that the classification of finite simple groups (CFSG) is complete. Our purpose is in con- structions which we re-examine in the light of observations that suggest that a substantial amount of insight is to be gained if we pursue novel connections to other, apparently disparate, areas of mathematics. This may lead to a natural home for the 26 sporadic simple groups which today are considered the complement of the Lie-Chevalley groups. 2 Overview of the Field In order to understand the importance of the new ideas and conjectures linked with Monstrous Moon- shine (MM) that we set out to develop, we have to understand its history, see [15, 19, 20]. Although the Monster is the most spectacular of the sporadic groups, it is just one of 26 groups under our wing. We discern three major evolutionary periods linked with the Monster group, the early and foundational one [5, 6, 7, 9, 10, 11, 17, 18, 22, 23], the time when the fruits of previous labour could be picked, cul- minating in Borcherds’ Fields medal rewarded proof of the conjecture [2], and finally the post Moonshine one, where it is becoming evident that we are not dealing with one particular isolated phenomenon but rather with a (possible) new class of objects of which MM is the most prominent representative so far, and its new mathematical connections [16]. An electronic collection of relevant articles for the subject has been posted at: http://www.fields.utoronto.ca/˜jplazas/MoonshineRoadmap.html 3 Recent Developments and Open Problems During the focused research group various parts of this picture became clearer. -
Modular Forms in String Theory and Moonshine
(Mock) Modular Forms in String Theory and Moonshine Miranda C. N. Cheng Korteweg-de-Vries Institute of Mathematics and Institute of Physics, University of Amsterdam, Amsterdam, the Netherlands Abstract Lecture notes for the Asian Winter School at OIST, Jan 2016. Contents 1 Lecture 1: 2d CFT and Modular Objects 1 1.1 Partition Function of a 2d CFT . .1 1.2 Modular Forms . .4 1.3 Example: The Free Boson . .8 1.4 Example: Ising Model . 10 1.5 N = 2 SCA, Elliptic Genus, and Jacobi Forms . 11 1.6 Symmetries and Twined Functions . 16 1.7 Orbifolding . 18 2 Lecture 2: Moonshine and Physics 22 2.1 Monstrous Moonshine . 22 2.2 M24 Moonshine . 24 2.3 Mock Modular Forms . 27 2.4 Umbral Moonshine . 31 2.5 Moonshine and String Theory . 33 2.6 Other Moonshine . 35 References 35 1 1 Lecture 1: 2d CFT and Modular Objects We assume basic knowledge of 2d CFTs. 1.1 Partition Function of a 2d CFT For the convenience of discussion we focus on theories with a Lagrangian description and in particular have a description as sigma models. This in- cludes, for instance, non-linear sigma models on Calabi{Yau manifolds and WZW models. The general lessons we draw are however applicable to generic 2d CFTs. An important restriction though is that the CFT has a discrete spectrum. What are we quantising? Hence, the Hilbert space V is obtained by quantising LM = the free loop space of maps S1 ! M. Recall that in the usual radial quantisation of 2d CFTs we consider a plane with 2 special points: the point of origin and that of infinity. -
JHEP09(2009)052 July 14, 2009 S, Extended : August 30, 2009 : September 9, 2009 Alize, When Com- : Received Eneralized S-Rule
Published by IOP Publishing for SISSA Received: July 14, 2009 Accepted: August 30, 2009 Published: September 9, 2009 Webs of five-branes and N = 2 superconformal field JHEP09(2009)052 theories Francesco Benini,a Sergio Benvenutia and Yuji Tachikawab aDepartment of Physics, Princeton University, Washington Road, Princeton NJ 08544, U.S.A. bSchool of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton NJ 08540, U.S.A. E-mail: [email protected], [email protected], [email protected] Abstract: We describe configurations of 5-branes and 7-branes which realize, when com- pactified on a circle, new isolated four-dimensional N = 2 superconformal field theories recently constructed by Gaiotto. Our diagrammatic method allows to easily count the dimensions of Coulomb and Higgs branches, with the help of a generalized s-rule. We furthermore show that superconformal field theories with E6,7,8 flavor symmetry can be analyzed in a uniform manner in this framework; in particular we realize these theories at infinitely strongly-coupled limits of quiver theories with SU gauge groups. Keywords: Supersymmetry and Duality, Brane Dynamics in Gauge Theories, Extended Supersymmetry, Intersecting branes models ArXiv ePrint: 0906.0359 c SISSA 2009 doi:10.1088/1126-6708/2009/09/052 Contents 1 Introduction 1 2 N-junction and T [AN−1] theory 4 2.1 N-junction 4 2.2 Coulomb branch 6 2.3 Higgs branch 6 JHEP09(2009)052 2.4 Dualities and Seiberg-Witten curve 7 3 General punctures and the s-rule 8 3.1 Classification of punctures 8 3.2 Generalized