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Mathieu moonshine and σ-models on K3
Roberto Volpato
Albert-Einstein-InstituteMax-Planck-Institut fur Gravitationsphysik
Potsdam, Golm
Algebra, Geometry and Physics of BPS StatesBonn, 12 November 2012
ReferencesM.R.Gaberdiel, R.Volpato, 1206.5143 [hep-th]
M.R.Gaberdiel, S.Hohenegger, R.Volpato, 1106.4315, 1008.3778, 1006.0221 [hep-th]
Works in progress: M.R.Gaberdiel, D.Persson, H.Ronellenfitsch, R.Volpato
M24 and K3 models Roberto Volpato AEI Potsdam
Monstrous Moonshine
Consider PSL(2,Z)-invariant J-function (q = e2πiτ):
J(τ) = q−1 + 196884q + 21493760q2 + 864299970q3 + . . .
Coefficients are dimension of reps of Monster group M [McKay]:
J(τ) =∞∑
n=−1
qn dimVn
Vn ≡ representations of M
McKay-Thompson series: Tg (τ) =∑∞
n=−1 qn TrVn(g), for each g ∈M
J(τ) is the partition function of a chiral CFT V \ (c = 24)with symmetry group M[Frenkel, Lepowski, Meurman ’88]
J(τ) = TrV \(qL0−c24 )
M24 and K3 models Roberto Volpato AEI Potsdam
Monstrous Moonshine
Modular invariant function J
Monster group M
???
Monster module V \
Partition function
Symmetry Group
M24 and K3 models Roberto Volpato AEI Potsdam
Monstrous Moonshine
Modular invariant function J
Monster group M
???
Monster module V \
Partition function
Symmetry Group
M24 and K3 models Roberto Volpato AEI Potsdam
Mathieu Moonshine
Elliptic genus of K3
Mathieu group M24
???
Non-linear σ-models on K3
(Refined) Partition function
?????×
M24 and K3 models Roberto Volpato AEI Potsdam
Mathieu Moonshine
Elliptic genus of K3
Mathieu group M24
??? Non-linear σ-models on K3
(Refined) Partition function
?????
×
M24 and K3 models Roberto Volpato AEI Potsdam
Mathieu Moonshine
Elliptic genus of K3
Mathieu group M24
??? Non-linear σ-models on K3
(Refined) Partition function
?????
×
M24 and K3 models Roberto Volpato AEI Potsdam
Plan of the talk
1 Definitions and EOT conjecture
2 Twining genera
3 Symmetries of K3 models
4 Torus orbifolds and exceptional K3 models
5 Conclusions and open questions
M24 and K3 models Roberto Volpato AEI Potsdam
The group M24
M24 is a finite simple group of order
|M24| = 210 · 33 · 5 · 7 · 11 · 23 ∼ 2× 108
Properties:
Subgroup of S24(=permutations of 24 symbols)
Group of automorphisms of Niemeier lattice A241 /Weyl reflections
26 conjugacy classes
26 irreducible representations of dimensions
1, 23, 45, 231, 252, 253, 483, 770, 990, 1035, 1265,
1771, 2024, 2277, 3312, 3520, 5313, 5544, 5796, 10395
M24 and K3 models Roberto Volpato AEI Potsdam
Elliptic genus: definition
dim = 2 SuperCFT N = (4, 4) with central charge c = 6
Non-linear σ-models with target space K3
The model depends on the choice of metric and B-field(moduli space of theories).
Elliptic genus
φK3(τ, z) = TrRR((−1)F+F qL0−
c24 qL0−
c24 y2J
30)
where q = e2πiτ, y = e2πiz .
J30 is the 3rd comp of (left) su(2) in N = (4, 4) SC algebra
M24 and K3 models Roberto Volpato AEI Potsdam
Elliptic genus: properties
φK3(τ, z) = TrRR((−1)F+F qL0−
c24 qL0−
c24 y2J
30)
Independent of the moduli (metric and B-field)
Holomorphic in τ and z
Quasi-periodicity and modular properties:
φK3(τ, z + `τ+ `′) = e−2πi(`2τ+2`z)φ(τ, z) `, ` ′ ∈ Z
φK3
( aτ+ b
cτ+ d,
z
cτ+ d
)= e2πi
cz2
cτ+d φ(τ, z)
(a bc d
)∈ SL(2,Z)
≡ (weak) Jacobi form of weight 0 and index 1
φK3(τ, z = 0) = Euler number of K3 = 24
M24 and K3 models Roberto Volpato AEI Potsdam
Distinct unitary RR reps of N = 4 at c = 6 labeled by
(h, `) = Eigenvalues under (L0, J30 ) of the highest weight state
(h, `) = (14 , 0)BPS ; (14 ,12)BPS ; (14 + 1, 12), (
14 + 2, 12), . . .
Only states at h = 14 (right-moving ground states) contribute to φK3
Decomposition of φK3 into left N = 4 characters at c = 6
φK3(τ, z) =∑(h,`)
Ah,` chh,`(τ, z)
where
chh,`(τ, z) = Tr(h,`)((−1)2J
30 qL0−
c24 y2J
30)
Ah,` is (graded) multiplicity of (h, `) rep
M24 and K3 models Roberto Volpato AEI Potsdam
EOT observation
Multiplicities of (massive) N = 4 reps:
12Ah,` = 45, 231, 770, 2277, 5796, 13915, . . .
Dimensions of irreps of M24:
1, 23, 45, 231, 252, 253, 483, 770, 990, 1035, 1265,1771, 2024, 2277, 3312, 3520, 5313, 5544, 5796, 10395
. . . and 13915 = 3520 + 10395(for higher h, many possible decompositions ⇒ ambiguity)[Eguchi, Ooguri, Tachikawa 1004.0956]
Conjecture: There is an action of M24 on the space of states contributingto the K3 elliptic genus
M24 and K3 models Roberto Volpato AEI Potsdam
A Mathieu Moonshine?
Ah,` are the dimensions of reps Rh,` of Mathieu group M24
φK3(τ, z) =∑(h,`)
dimRh,` chN=4h,` (τ, z)
We can define the twining genera[Cheng 1005.5415; Gaberdiel, Hohenegger, R.V. 1006.0221]
φg (τ, z) =TrRR(g (−1)F+FqL0−
c24 qL0−
c24 y2J
30), g ∈ M24
=∑(h,`)
TrRh,`(g) chN=4
h,` (τ, z)
In Monster Moonshine, the analogous objects are McKay-Thompson series
M24 and K3 models Roberto Volpato AEI Potsdam
A Mathieu Moonshine?
If g commutes with N = (4, 4) SConf symmetry↓φg must be a weak Jacobi form under (N = ord(g))
Γ0(N) :={(
a bc d
)∈ SL(2,Z) | c ≡ 0 mod N
}⊂ SL(2,Z)
We should also allow for a non-trivial multiplier system[ Gaberdiel, Hohenegger, R.V. 1008.3778]:
φg
( aτ+ b
cτ+ d,
z
cτ+ d
)= χg
(a bc d
)e2πi
cz2
cτ+d φg (τ, z)(a bc d
)∈ Γ0(N)
where χg : Γ0(N)→ U(1)
(Similar to what happens with McKay-Thompson series)
M24 and K3 models Roberto Volpato AEI Potsdam
Results
For each M24 conjugacy class g there is a function φg (τ, z) such that
1 φe(τ, z) (e ≡ identity in M24) is the elliptic genus of K3
2 φg is a weak Jacobi form for Γ0(N), N = order of g
3 There are non-trivial M24-representations Rh,`
φg (τ, z) =∑(h,`)
TrRh,`(g) chN=4
h,` (τ, z)
The representations Rh,` with these properties are unique(but the surprising fact is existence rather than uniqueness...)
[Gaberdiel, Hohenegger, R.V. 1008.3778; Eguchi, Hikami 1008.4924; Gannon]
M24 and K3 models Roberto Volpato AEI Potsdam
Mathieu Moonshine
Elliptic genus of K3
Mathieu group M24
??? Non-linear σ-models on K3
(Refined) Partition function
????
M24 and K3 models Roberto Volpato AEI Potsdam
A relation between K3 and Mathieu groups
A theorem in algebraic geometry gives a connection between K3 andMathieu groups
Mukai Theorem
Finite groups of symplectic automorphisms of K3 surf’s are subgroups ofM23 ⊆ M24.[Mukai 1988; Kondo 1998]
A symplectic automorphism of the K3 target space inducesa symmetry of the corresponding σ-model.
But σ-models may have non-geometrical (quantum) symmetries
Can we classify the groups of discrete symmetries of K3 σ-models?(Quantum analogue of Mukai theorem)
M24 and K3 models Roberto Volpato AEI Potsdam
Classification Theorem
Let Co0 be the group of automorphisms of the Leech lattice Λ(even self-dual lattice of dim 24 with no elements of norm 2)
Let G be a group of symmetries of a K3 σ-model that commute withN = (4, 4) and spectral flow.
Theorem
G is a subgroup of Co0 ≡ Aut(Λ) fixing pointwise a sublattice of Λof rank at least 4.
Conversely, any G ⊂ Co0 fixing a sublattice of Λ of rank at least 4 is thesymmetry group of some K3 model.
[Gaberdiel, Hohenegger, R.V. 1106.4315]
Also M24 is a subgroup of Co0, but...
M24 and K3 models Roberto Volpato AEI Potsdam
Subgroups G ⊂ Co0 fixing a sublattice of rank 4:
G ⊂ Z122 oM24 (at least 4 orbits on 24-dim rep)
G = 51+2.Z4
G = Z43 o A6 or G = 31+4.Z2.G
′′ with G ′′ = 1,Z2 or Z22
What can we learn from this description?
There is no G such that M24 ⊆ G
There are some G such that G 6⊂ M24
M24 and K3 models Roberto Volpato AEI Potsdam
Sketch of the proof
Known facts about σ-models on K3:[Aspinwall 9611375, Nahm, Wendland 9912067]
There are 24 RR ground states at h = h = 14 (≡ R4,20)
The ground states are contained in N = (4, 4) supermultiplets:
4 are in one (h, `; h, ¯) = ( 14 ,12 ;
14 ,
12 ) (subspace Π ⊂ R4,20)
20 are in 20 distinct (h, `; h, ¯) = ( 14 , 0;14 , 0)
The D-brane charges form an even self-dual lattice Γ4,20
We can think of Γ4,20 as embedded in (the dual of) R4,20
Moduli space of K3 models:
O(Γ4,20)\O(4, 20,R)/(O(4,R)× O(20,R))
M24 and K3 models Roberto Volpato AEI Potsdam
Sketch of the proof
G : group of symmetries that commute with N = (4, 4) and spectral flow
1 G acts faithfully on the lattice Γ4,20 ⊂ R4,20
2 G fixes pointwise Π ⊂ R4,20, with dimΠ = 4
3 G acts faithfully on the sublattice L = Γ4,20 ∩ Π⊥ with dim L ≤ 20
4 L can be embedded into the Leech Λ and the action of G extends toautomorphisms of Λ
5 The sublattice ΛG ⊂ Λ of vectors fixed by G is the orthogonalcomplement of L ⊂ Λ ↓
G is a subgroup of Aut(Λ) ≡ Co0 that fixes a sublattice of rank≥ 4
M24 and K3 models Roberto Volpato AEI Potsdam
Discussion
Problems:
1 There are no K3 σ-models with symmetry group M24
2 There are groups of symmetries G 6⊂M24 (exceptional cases)
3 All groups are contained in Co0 but no Conway Moonshine
Open questions:
Are there unknown SCFTs with the same elliptic genus?
Is M24 the symmetry of some different ‘structure’ related to K3?
Are exceptional models in some sense ‘special’?
Exceptional models seem related to orbifolds of non-linear σ models on T 4
[Gaberdiel, R.V. 1206.5143]
M24 and K3 models Roberto Volpato AEI Potsdam
Cyclic torus orbifolds
CFT orbifold Given a CFT C with a symmetry g , project on g -invariantstates and introduce new (twisted) sectors
(Cyclic) Torus orbifoldsSpecial families of K3 models are given by orbifolds (in CFT sense)of non-linear σ-models on T 4 by some Zn group of symmetries
Easiest example: non-linear σ-model with target space T 4/ZN ,where ZN is a group of automorphisms of T 4
In general, group ZN might be non-geometric symmetry(e.g. asymmetric orbifolds)
M24 and K3 models Roberto Volpato AEI Potsdam
Results I
Classification of orbifolds of T 4 models:
Symmetric (geometric) orbifolds with ord(g) = 2, 3, 4, 6 (known)
Asymmetric orbifolds with ord(g) = 4, 5, 6, 8, 10, 12 (NEW!)
Explicitly constructed C/g for ord(g) = 5[Gaberdiel, R.V. 1206.5143]
M24 and K3 models Roberto Volpato AEI Potsdam
Results II
Results
1 All torus orbifolds are exceptional
2 Most exceptional models are torus orbifolds.
(a) G ⊂ Z122 oM24 (at least 4 orbits on 24-dim rep)
(b) G = 51+2.Z4
(c) G = Z43 o A6 or G = 31+4.Z2.G
′′ with G ′′ = 1,Z2 or Z22
In particular:
case (b) ⇔ Z5 orbifold of T 4 model
case (c) ⇔ Z3 orbifold of T 4 model
[Gaberdiel, R.V. 1206.5143]
M24 and K3 models Roberto Volpato AEI Potsdam
Conclusions and open questions
Strong evidence of a Mathieu moonshine
Interpretation in terms of non-linear σ-model is problematic
More and more evidence that there is a CFT behind it:even the Generalised Moonshine works! (see Daniel’s talk)
Many open questions:
Analog of genus zero property of Montrous Moonshine?[Cheng, Duncan]
Relation with the old M24 η-product Moonshine? [Mason]
Relation with the Umbral Moonshine? [Cheng, Duncan, Harvey]
M24-moonshine in ‘second quantized’ string on K3?
M24 and K3 models Roberto Volpato AEI Potsdam