K3 Surfaces, Mathieu Moonshine, and Quantum Codes Gregory Moore Rutgers
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Generating the Mathieu Groups and Associated Steiner Systems
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Discrete Mathematics 112 (1993) 41-47 41 North-Holland Generating the Mathieu groups and associated Steiner systems Marston Conder Department of Mathematics and Statistics, University of Auckland, Private Bag 92019, Auckland, New Zealand Received 13 July 1989 Revised 3 May 1991 Abstract Conder, M., Generating the Mathieu groups and associated Steiner systems, Discrete Mathematics 112 (1993) 41-47. With the aid of two coset diagrams which are easy to remember, it is shown how pairs of generators may be obtained for each of the Mathieu groups M,,, MIz, Mz2, M,, and Mz4, and also how it is then possible to use these generators to construct blocks of the associated Steiner systems S(4,5,1 l), S(5,6,12), S(3,6,22), S(4,7,23) and S(5,8,24) respectively. 1. Introduction Suppose you land yourself in 24-dimensional space, and are faced with the problem of finding the best way to pack spheres in a box. As is well known, what you really need for this is the Leech Lattice, but alas: you forgot to bring along your Miracle Octad Generator. You need to construct the Leech Lattice from scratch. This may not be so easy! But all is not lost: if you can somehow remember how to define the Mathieu group Mz4, you might be able to produce the blocks of a Steiner system S(5,8,24), and the rest can follow. In this paper it is shown how two coset diagrams (which are easy to remember) can be used to obtain pairs of generators for all five of the Mathieu groups M,,, M12, M22> Mz3 and Mz4, and also how blocks may be constructed from these for each of the Steiner systems S(4,5,1 I), S(5,6,12), S(3,6,22), S(4,7,23) and S(5,8,24) respectively. -
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. -
Sphere Packing, Lattice Packing, and Related Problems
Sphere packing, lattice packing, and related problems Abhinav Kumar Stony Brook April 25, 2018 Sphere packings Definition n A sphere packing in R is a collection of spheres/balls of equal size which do not overlap (except for touching). The density of a sphere packing is the volume fraction of space occupied by the balls. ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ In dimension 1, we can achieve density 1 by laying intervals end to end. In dimension 2, the best possible is by using the hexagonal lattice. [Fejes T´oth1940] Sphere packing problem n Problem: Find a/the densest sphere packing(s) in R . In dimension 2, the best possible is by using the hexagonal lattice. [Fejes T´oth1940] Sphere packing problem n Problem: Find a/the densest sphere packing(s) in R . In dimension 1, we can achieve density 1 by laying intervals end to end. Sphere packing problem n Problem: Find a/the densest sphere packing(s) in R . In dimension 1, we can achieve density 1 by laying intervals end to end. In dimension 2, the best possible is by using the hexagonal lattice. [Fejes T´oth1940] Sphere packing problem II In dimension 3, the best possible way is to stack layers of the solution in 2 dimensions. This is Kepler's conjecture, now a theorem of Hales and collaborators. mmm m mmm m There are infinitely (in fact, uncountably) many ways of doing this! These are the Barlow packings. Face centered cubic packing Image: Greg A L (Wikipedia), CC BY-SA 3.0 license But (until very recently!) no proofs. In very high dimensions (say ≥ 1000) densest packings are likely to be close to disordered. -
ORBITS in the LEECH LATTICE 1. Introduction the Leech Lattice Λ Is a Lattice in 24-Dimensional Euclidean Space with Many Remark
ORBITS IN THE LEECH LATTICE DANIEL ALLCOCK Abstract. We provide an algorithm for determining whether two vectors in the Leech lattice are equivalent under its isometry group, 18 the Conway group Co 0 of order 8 10 . Our methods rely on and develop the work of R. T.∼ Curtis,× and we describe our in- tended applications to the symmetry groups of Lorentzian lattices and the enumeration of lattices of dimension 24 with good prop- erties such as having small determinant. Our≈ algorithm reduces 12 the test of equivalence to 4 tests under the subgroup 2 :M24, ≤ and a test under this subgroup to 12 tests under M24. We also give algorithms for testing equivalence≤ under these two subgroups. Finally, we analyze the performance of the algorithm. 1. Introduction The Leech lattice Λ is a lattice in 24-dimensional Euclidean space with many remarkable properties, for us the most important of which is that its isometry group (modulo I ) is one of the sporadic finite {± } simple groups. The isometry group is called the Conway group Co 0, and our purpose is to present an algorithm for a computer to determine whether two given vectors of Λ are equivalent under Co 0. The group is fairly large, or order > 8 1018, so the obvious try-every-isometry algorithm is useless. Instead,× we use the geometry of Λ to build a faster algorithm; along the way we build algorithms for the problem 24 12 of equivalence of vectors in R under the subgroups 2 :M24 and M24, where M24 is the Mathieu group permuting the 24 coordinates. -
Optimality and Uniqueness of the Leech Lattice Among Lattices
ANNALS OF MATHEMATICS Optimality and uniqueness of the Leech lattice among lattices By Henry Cohn and Abhinav Kumar SECOND SERIES, VOL. 170, NO. 3 November, 2009 anmaah Annals of Mathematics, 170 (2009), 1003–1050 Optimality and uniqueness of the Leech lattice among lattices By HENRY COHN and ABHINAV KUMAR Dedicated to Oded Schramm (10 December 1961 – 1 September 2008) Abstract We prove that the Leech lattice is the unique densest lattice in R24. The proof combines human reasoning with computer verification of the properties of certain explicit polynomials. We furthermore prove that no sphere packing in R24 can 30 exceed the Leech lattice’s density by a factor of more than 1 1:65 10 , and we 8 C give a new proof that E8 is the unique densest lattice in R . 1. Introduction It is a long-standing open problem in geometry and number theory to find the densest lattice in Rn. Recall that a lattice ƒ Rn is a discrete subgroup of rank n; a minimal vector in ƒ is a nonzero vector of minimal length. Let ƒ vol.Rn=ƒ/ j j D denote the covolume of ƒ, i.e., the volume of a fundamental parallelotope or the absolute value of the determinant of a basis of ƒ. If r is the minimal vector length of ƒ, then spheres of radius r=2 centered at the points of ƒ do not overlap except tangentially. This construction yields a sphere packing of density n=2 r Án 1 ; .n=2/Š 2 ƒ j j since the volume of a unit ball in Rn is n=2=.n=2/Š, where for odd n we define .n=2/Š .n=2 1/. -
Octonions and the Leech Lattice
Octonions and the Leech lattice Robert A. Wilson School of Mathematical Sciences, Queen Mary, University of London, Mile End Road, London E1 4NS 18th December 2008 Abstract We give a new, elementary, description of the Leech lattice in terms of octonions, thereby providing the first real explanation of the fact that the number of minimal vectors, 196560, can be expressed in the form 3 × 240 × (1 + 16 + 16 × 16). We also give an easy proof that it is an even self-dual lattice. 1 Introduction The Leech lattice occupies a special place in mathematics. It is the unique 24- dimensional even self-dual lattice with no vectors of norm 2, and defines the unique densest lattice packing of spheres in 24 dimensions. Its automorphism group is very large, and is the double cover of Conway’s group Co1 [2], one of the most important of the 26 sporadic simple groups. This group plays a crucial role in the construction of the Monster [13, 4], which is the largest of the sporadic simple groups, and has connections with modular forms (so- called ‘Monstrous Moonshine’) and many other areas, including theoretical physics. The book by Conway and Sloane [5] is a good introduction to this lattice and its many applications. It is not surprising therefore that there is a huge literature on the Leech lattice, not just within mathematics but in the physics literature too. Many attempts have been made in particular to find simplified constructions (see for example the 23 constructions described in [3] and the four constructions 1 described in [15]). -
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. -
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. -
A Uniform Construction of the Holomorphic Voas of Central
A Uniform Construction of the 71 Holomorphic VOAs of c = 24 from the Leech Lattice Sven Möller (joint work with Nils Scheithauer) Vertex Operator Algebras, Number Theory, and Related Topics: A Conference in Honor of Geoffrey Mason, California State University, Sacramento 12th June 2018 Schellekens’ List Orbifold Construction and Dimension Formulae A Generalised Deep-Hole Construction Contents 1 Schellekens’ List 2 Orbifold Construction and Dimension Formulae 3 A Generalised Deep-Hole Construction Sven Möller A Uniform Construction of the 71 holomorphic VOAs of c = 24 Schellekens’ List Orbifold Construction and Dimension Formulae A Generalised Deep-Hole Construction Holomorphic VOAs of Small Central Charge Proposition (Consequence of [Zhu96]) Let V be a strongly rational, holomorphic VOA. Then the central charge c of V is in 8Z≥0. + c = 8: VE8 , c = 16: V 2 , V (only lattice theories) [DM04] E8 D16 Theorem ([Sch93, DM04, EMS15]) Let V be a strongly rational, holomorphic VOA of central charge c = 24. Then the Lie algebra V1 is isomorphic to one of the 71 Lie algebras on Schellekens’ list (V \, 24 Niemeier lattice theories, etc. with chV (τ) = j(τ) − 744 + dim(V1)). c = 32: already more than 1 160 000 000 lattice theories Sven Möller A Uniform Construction of the 71 holomorphic VOAs of c = 24 Schellekens’ List Orbifold Construction and Dimension Formulae A Generalised Deep-Hole Construction Classification Orbifold constructions give all 71 cases on Schellekens’ list. [FLM88, DGM90, Don93, DGM96, Lam11, LS12, LS15, Miy13, SS16, EMS15, Mö16, LS16b, LS16a, LL16] Theorem (Classification I) There is a strongly rational, holomorphic VOA V of central charge c = 24 with Lie algebra V1 if and only if V1 is isomorphic to one of the 71 Lie algebras on Schellekens’ list. -
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. -
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.