Mathieu Moonshine and Orbifold K3s
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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. -
Mock Moonshine by Prof. Kishore Marathe City University of New
Mock Moonshine by Prof. Kishore Marathe City University of New York, Brooklyn College International Conference on Recebt Developments in String Theory Congressi Stefano Franscini - Monte Verita, Switzerland July 21 to 25, 2014 ====================== 1 Thirty years ago some very surprising relations between the Fourier coefficients of the Jacobi Hauptmodul or the J-function and represen- tations of the largest finite simple sporadic group, the Monster were discovered. Precise formulation of these relations is now called the ’Monstrous Moonshine’. It has given rise to a large body of new mathematics. The moonshine correspondence has been extended to other groups revealing unexpected relations to conformal field theory, gravity and string theory in physics and to Ramanujan’s mock theta functions and its extensions in mathe- matics. We call these results which have been discoverd in the last 30 years ’ Mock Moon- shine’. We will survey some recent develop- ments related to Mock Moonshine and indicate directions for future research. 2 List of Topics 1. Some Historical Remarks 2. Modular objects 3. Monstrous Moonshine Conjectures 4. Monstrous Moonshine and Vertex Algebras 5. Moonshine for other groups 6. Mock Moonshine and Field Theories 3 The following historical material is taken from [4]. Recall that a group is called simple if it has no proper non-trivial normal subgroup. Thus an abelian group is simple if and only if it is isomorphic to one of the groups Zp, for p a prime number. This is the simplest example of an infinite family of finite simple groups. An- other infinite family of finite simple groups is the family of alternating groups An,n> 4 that we study in the first course in algebra. -
Construction of an Umbral Module
Thank the Organizers Construction of an Umbral module With John Duncan J. Harvey, Eurostrings 2015 OUTLINE 1. Moonshine, Monstrous and Umbral 2. A free fermion trick 3. The 3E8 example of Umbral Moonshine 4. Indefinite lattice theta functions 5. A Vertex Operator Algebra for indefinite lattices 6. Putting the pieces together 7. What does it mean for string theory? M O O N S H I N E M (Mock)ModularForms G S Groups (Finite) String theory A Algebras (VOA) The original example of this structure is Monstrous Moonshine G The Monster sporadic group M The weight zero modular function 1 2⇡i⌧ J(⌧)=q− + 196884q + ,q= e ··· A Vertex Operator Algebra (OPE of chiral Vertex operators) S Bosonic or Heterotic String on an asymmetric orbifold background 24 (R /ΛL)/(Z/2) We now have Mathieu Moonshine and its extension to Umbral Moonshine. We know the extension for two of these objects: G : M24 or more generally GX = Aut(LX )/W X M : A weight 1/2 mock modular form whose coefficients count the multiplicities of massive Eguchi, N=4 SCA characters in the elliptic genus of K3 Ooguri, Tachikawa (2) 1/8 2 3 H (⌧)=2q− 1 + 45q + 231q + 770q + − ··· or more generally, a weight 1/2, m-1 component X vector-valued mock modular form Hr (⌧) Here L X is one of the 23, rank 24 Niemeier lattices and m = m ( X ) is its Coxeter number. Are there analogs of the VOA algebraic structure and/or a string theoretic interpretation of these structures? More specifically, is there an explicit construction of the infinite-dimensional G X modules implied by these constructions along with an explicit action of G X ? That is, the M24 mock modular form suggests that there exists an infinite set of vector spaces (2) (2) (2) K 1/8,K7/8,K15/8, − ··· of dimension 2, 2x45, 2x231, …that provide representations of M24 and should be combined into (2) (2) 1 K = n=0 Kn 1/8 − L In Monstrous Moonshine we have \ V = Vn n 1 M≥− 1 n dimVn = c(n),J(q)= c(n)q n= 1 X− with V n the vector space of states of conformal dimension n c/ 24 in the Monster CFT. -
A Classification of Clifford Algebras As Images of Group Algebras of Salingaros Vee Groups
DEPARTMENT OF MATHEMATICS TECHNICAL REPORT A CLASSIFICATION OF CLIFFORD ALGEBRAS AS IMAGES OF GROUP ALGEBRAS OF SALINGAROS VEE GROUPS R. Ablamowicz,M.Varahagiri,A.M.Walley November 2017 No. 2017-3 TENNESSEE TECHNOLOGICAL UNIVERSITY Cookeville, TN 38505 A Classification of Clifford Algebras as Images of Group Algebras of Salingaros Vee Groups Rafa lAb lamowicz, Manisha Varahagiri and Anne Marie Walley Abstract. The main objective of this work is to prove that every Clifford algebra C`p;q is R-isomorphic to a quotient of a group algebra R[Gp;q] modulo an ideal J = (1 + τ) where τ is a central element of order 2. p+q+1 Here, Gp;q is a 2-group of order 2 belonging to one of Salingaros isomorphism classes N2k−1;N2k; Ω2k−1; Ω2k or Sk. Thus, Clifford al- gebras C`p;q can be classified by Salingaros classes. Since the group algebras R[Gp;q] are Z2-graded and the ideal J is homogeneous, the quotient algebras R[G]=J are Z2-graded. In some instances, the isomor- ∼ phism R[G]=J = C`p;q is also Z2-graded. By Salingaros Theorem, the groups Gp;q in the classes N2k−1 and N2k are iterative central products of the dihedral group D8 and the quaternion group Q8, and so they are extra-special. The groups in the classes Ω2k−1 and Ω2k are central products of N2k−1 and N2k with C2 × C2, respectively. The groups in the class Sk are central products of N2k or N2k with C4. Two algorithms to factor any Gp;q into an internal central product, depending on the class, are given. -
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. -
String Theory Moonshine
Strings 2014, Princeton Umbral Moonshine and String Theory Miranda Cheng University of Amsterdam* *: on leave from CNRS, France. A Myseros Story Abot Strings on K3 Finite Moonshine Modular Groups Objects symmetries of interesting objects functions with special symmetries K3 Sigma-Model 2d sigma models: use strings to probe the geometry. M = K3 Σ N=(4,4) superconformal Elliptic Genus of 2d SCFT In a 2d N>=(2,2) SCFT, susy states are counted by the elliptic genus: q = e2⇡i⌧ ,y = e2⇡iz • holomorphic [Schellekens–Warner, Witten ’87] • modular SL(2,Z) •topological EG = EG ⇣ ⌘ ⇣ ⌘ K3 Sigma-Model 2d sigma model on K3 is a N=(4,4) SCFT. ⇒ The spectrum fall into irred. representations of the N=4 SCA. 4 2 J +J¯ J L c/24 L c/24 ✓i(⌧,z) EG(⌧,z; K3) = Tr ( 1) 0 0 y 0 q 0− q¯ 0− =8 HRR − ✓ (⌧, 0) i=2 i ⇣ ⌘ X ✓ ◆ = 24 massless multiplets + tower of massive multiplets 1 2 ✓ (⌧,z) 1/8 2 3 = 1 24 µ(⌧,z)+2 q− ( 1 + 45 q + 231 q + 770 q + ...) ⌘3(⌧) − “Appell–Lerch⇣ sum” numbers of massive N=4 multiplets ⌘ also dimensions of irreps of M24, ! an interesting finite group with ~108 elements [Eguchi–Ooguri–Tachikawa ’10] Why EG(K3) ⟷ M24? Q: Is there a K3 surface M whose symmetry (that preserves the hyperKähler structure) is M24? [Mukai ’88, Kondo ’98] No! M24 elements symmetries of M2 symmetries of M1 Q: Is there a K3 sigma model whose symmetry is M24? [Gaberdiel–Hohenegger–Volpato ’11] No! M24 elements possible symmetries of K3 sigma models 3. -
On Sylow 2-Subgroups of Finite Simple Groups of Order up to 210
ON SYLOW 2-SUBGROUPS OF FINITE SIMPLE GROUPS OF ORDER UP TO 210 DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Sergey Malyushitsky, M.S. ***** The Ohio State University 2004 Dissertation Committee: Approved by Professor Koichiro Harada, Adviser Professor Akos Seress Adviser Professor Ronald Solomon Department of Mathematics ABSTRACT A 2-group ( a group of order a power of 2 ) is called realizable if it occurs as a Sylow 2-subgroup of a finite simple group. The purpose of this thesis is to study all realizable groups of order up to 210. From the classification of all simple groups of finite order we know all realizable groups of order up to 210 as Sylow 2-subgroups of known finite simple groups. However without the use of classification determining all realizable 2-groups is very difficult. In the first part of the thesis we present an argument that produces all realizable groups of order up to 32, by eliminating one by one all 2-groups that can not occur as a Sylow 2-subgroup of a finite simple group. When the number of 2-groups of given order becomes too large to handle it by hand we attempt to use a computer for repetitive checks on a large number of 2-groups. The second part of the thesis is devoted to describing all realizable 2-groups of order up to 210 using the classification of all finite simple groups. We determine the identification number of each group in the Small Groups Library in GAP4 and compute the power-commutator presentation of each realizable group S of type G. -
K3 Elliptic Genus and an Umbral Moonshine Module
UvA-DARE (Digital Academic Repository) K3 Elliptic Genus and an Umbral Moonshine Module Anagiannis, V.; Cheng, M.C.N.; Harrison, S.M. DOI 10.1007/s00220-019-03314-w Publication date 2019 Document Version Final published version Published in Communications in Mathematical Physics License CC BY Link to publication Citation for published version (APA): Anagiannis, V., Cheng, M. C. N., & Harrison, S. M. (2019). K3 Elliptic Genus and an Umbral Moonshine Module. Communications in Mathematical Physics, 366(2), 647-680. https://doi.org/10.1007/s00220-019-03314-w General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:27 Sep 2021 Commun. Math. Phys. 366, 647–680 (2019) Communications in Digital Object Identifier (DOI) https://doi.org/10.1007/s00220-019-03314-w Mathematical Physics K3 Elliptic Genus and an Umbral Moonshine Module Vassilis Anagiannis1, Miranda C. -
Umbral Moonshine and K3 Surfaces Arxiv:1406.0619V4 [Hep-Th] 18 Jul 2017
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:1406.0619v4 [hep-th] 18 Jul 2017 ∗[email protected] [email protected] zOn leave from CNRS, Paris. 1 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 49 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. -
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.