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Magical Supergravity Theories and Their Spectra Murat G¨ unaydin Aug. 4, 2011 Koc University, Istanbul M. G¨ unaydin, Istanbul,Aug. 4 2011 1

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Page 1: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Magical Supergravity Theories and Their Spectra

Murat Gunaydin

Aug. 4, 2011Koc University, Istanbul

M. Gunaydin, Istanbul,Aug. 4 2011 1

Page 2: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Review of magical supergravities in various dimensions.

I Gauging of 6d magical supergravities coupled tohypermultiplets

I Orbits of extremal BPS and non-BPS black hole solutions in5d and conformal extensions of U-duality groups as spectrumgenerating symmetry group.

I Orbits of extremal BPS and non-BPS black hole solutions in4d and quasiconformal extensions of U-duality groups asspectrum generating symmetry group.

I Minimal unitary realizations , quasiconformal groups andharmonic superspace

I Spectra of magical sugras and the minimal unitary realizationsof 3d U-duality groups.

I Open problems

M. Gunaydin, Istanbul,Aug. 4 2011 2

Page 3: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Bosonic part of the 5D Maxwell-Einstein supergravity Lagrangian(MESGT) MG, Sierra and Townsend (1983)

e−1L = −1

2R − 1

4

aIJF I

µνF Jµν − 1

2gxy (∂µϕ

x)(∂µϕy ) +

+e−1

6√

6CIJKε

µνρσλF IµνF J

ρσAKλ

coupling of (nV − 1) vector multiplets (Aaµ, λ

ai , ϕa) to N = 2

supergravity (gµν , ψiµ,Aµ) (I , J,K = 1, . . . , nV , i=1,2 , x, a = 1, . . . , (nV − 1) )

I 5D, N = 2 MESGT is uniquely determined by the constantsymmetric tensor CIJK .

I 5D MESGTs with symmetric scalar manifolds G/H such that G is asymmetry of the Lagrangian ⇐⇒ CIJK is given by the norm(determinant) N3 of a Euclidean Jordan algebra J of degree 3.

N3(J) = CIJKhIhJhK

M. Gunaydin, Istanbul,Aug. 4 2011 3

Page 4: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Bosonic part of the 5D Maxwell-Einstein supergravity Lagrangian(MESGT) MG, Sierra and Townsend (1983)

e−1L = −1

2R − 1

4

aIJF I

µνF Jµν − 1

2gxy (∂µϕ

x)(∂µϕy ) +

+e−1

6√

6CIJKε

µνρσλF IµνF J

ρσAKλ

coupling of (nV − 1) vector multiplets (Aaµ, λ

ai , ϕa) to N = 2

supergravity (gµν , ψiµ,Aµ) (I , J,K = 1, . . . , nV , i=1,2 , x, a = 1, . . . , (nV − 1) )

I 5D, N = 2 MESGT is uniquely determined by the constantsymmetric tensor CIJK .

I 5D MESGTs with symmetric scalar manifolds G/H such that G is asymmetry of the Lagrangian ⇐⇒ CIJK is given by the norm(determinant) N3 of a Euclidean Jordan algebra J of degree 3.

N3(J) = CIJKhIhJhK

M. Gunaydin, Istanbul,Aug. 4 2011 3

Page 5: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Bosonic part of the 5D Maxwell-Einstein supergravity Lagrangian(MESGT) MG, Sierra and Townsend (1983)

e−1L = −1

2R − 1

4

aIJF I

µνF Jµν − 1

2gxy (∂µϕ

x)(∂µϕy ) +

+e−1

6√

6CIJKε

µνρσλF IµνF J

ρσAKλ

coupling of (nV − 1) vector multiplets (Aaµ, λ

ai , ϕa) to N = 2

supergravity (gµν , ψiµ,Aµ) (I , J,K = 1, . . . , nV , i=1,2 , x, a = 1, . . . , (nV − 1) )

I 5D, N = 2 MESGT is uniquely determined by the constantsymmetric tensor CIJK .

I 5D MESGTs with symmetric scalar manifolds G/H such that G is asymmetry of the Lagrangian ⇐⇒ CIJK is given by the norm(determinant) N3 of a Euclidean Jordan algebra J of degree 3.

N3(J) = CIJKhIhJhK

M. Gunaydin, Istanbul,Aug. 4 2011 3

Page 6: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I There exist only four unified N = 2 Maxwell-Einstein Supergravitytheories in five dimensions with symmetric scalar manifolds. Theyare defined by the four simple Jordan algebras JA

3 of 3× 3Hermitian matrices over R,C,H and O. These magical supergravitytheories describe the coupling of 5, 8, 14 and 26 vector multiplets tosupergravity.

I Their scalar manifolds are the irreducible symmetric spaces

JR3 : M5 = SL(3,R)/SO(3)

JC3 : M5 = SL(3,C)/SU(3)

JH3 : M5 = SU∗(6)/USp(6)

JO3 : M5 = E6(−26)/F4

I The generic Jordan family defined by non-simple Jordan algebrasJ = Γ(1,n−1) ⊕ R with the scalar manifold

SO(n − 1, 1)× SO(1, 1)

SO(n − 1)

M. Gunaydin, Istanbul,Aug. 4 2011 4

Page 7: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I There exist only four unified N = 2 Maxwell-Einstein Supergravitytheories in five dimensions with symmetric scalar manifolds. Theyare defined by the four simple Jordan algebras JA

3 of 3× 3Hermitian matrices over R,C,H and O. These magical supergravitytheories describe the coupling of 5, 8, 14 and 26 vector multiplets tosupergravity.

I Their scalar manifolds are the irreducible symmetric spaces

JR3 : M5 = SL(3,R)/SO(3)

JC3 : M5 = SL(3,C)/SU(3)

JH3 : M5 = SU∗(6)/USp(6)

JO3 : M5 = E6(−26)/F4

I The generic Jordan family defined by non-simple Jordan algebrasJ = Γ(1,n−1) ⊕ R with the scalar manifold

SO(n − 1, 1)× SO(1, 1)

SO(n − 1)

M. Gunaydin, Istanbul,Aug. 4 2011 4

Page 8: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Symmetry Groups of Simple Jordan algebrasJ Rot(J) Lor(J) Conf (J)

JRn SO(n) SL(n,R) Sp(2n,R)

JCn SU(n) SL(n,C) SU(n, n)

JHn USp(2n) SU∗(2n) SO∗(4n)

JO3 F4 E6(−26) E7(−25)

Γ(1,d) SO(d) SO(d , 1) SO(d , 2)

Table: The complete list of simple Euclidean Jordan algebras and theirrotation ( automorphism), ”Lorentz” ( reduced structure) and”Conformal” ( linear fractional) groups. The symbols R, C, H, Orepresent the four division algebras. JA

n denotes a Jordan algebra of n× nhermitian matrices over A. Γ(1,d) denotes the Jordan algebra of Diracgamma matrices.

M. Gunaydin, Istanbul,Aug. 4 2011 5

Page 9: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Under dimensional reduction of 5D MESGT to 4D

M5 =Lor(J)

Rot(J)⇒ M4 =

Conf (J)

Lor(J)× U(1)

where Lor(J) is the compact real form of the Lorentz group ofJ. The bosonic sector of dimensionally reduced Lagrangian is

e−1L(4) = −1

2R − gI J(∂µz I )(∂µzJ)

+1

4Im(NAB)FA

µνFµνB − 1

8Re(NAB)εµνρσFA

µνFBρσ

In 5D: Vector fields AµI ⇔ Elements of Jordan algebra J

In 4D: FAµν ⊕ FA

µν ⇔ Elements of a Freudenthal triple system(FTS) F(J) :

X =

R J F 0µν F I

µν

⇔J R F I

µν F 0µν

M. Gunaydin, Istanbul,Aug. 4 2011 6

Page 10: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

N = 2 MESGTs reduce to N = 4 supersymmetric sigma modelscoupled to gravity in d = 3. The target manifolds of magicalsupergravity theories in d = 3 are the exceptional quaternionicsymmetric spaces:

IF4(4)

Usp(6)×USp(2) ,E6(2)

SU(6)×SU(2) ,E7(5)

SO(12)×SU(2) ,E8(−24)

E7×SU(2)

I The generic Jordan family of MESGT reduced to d = 3 havethe target spaces: SO(n+2,4)

SO(n+2)×SO(4)

Exceptional N = 2 versus Maximal N = 8 Supergravity:

I The exceptional N = 2 supergravity is defined by theexceptional Jordan algebra JO

3 of 3× 3 Hermitian matricesover real octonions. Its global invariance group in 5D isE6(−26) with maximal compact subgroup F4.

I In D = 4 and D = 3 the exceptional supergravity has E7(−25)

and E8(−24) as its U-duality group while the maximal N = 8supergravity has E7(7) and E8(8), respectively.

M. Gunaydin, Istanbul,Aug. 4 2011 7

Page 11: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

N = 2 MESGTs reduce to N = 4 supersymmetric sigma modelscoupled to gravity in d = 3. The target manifolds of magicalsupergravity theories in d = 3 are the exceptional quaternionicsymmetric spaces:

IF4(4)

Usp(6)×USp(2) ,E6(2)

SU(6)×SU(2) ,E7(5)

SO(12)×SU(2) ,E8(−24)

E7×SU(2)

I The generic Jordan family of MESGT reduced to d = 3 havethe target spaces: SO(n+2,4)

SO(n+2)×SO(4)

Exceptional N = 2 versus Maximal N = 8 Supergravity:

I The exceptional N = 2 supergravity is defined by theexceptional Jordan algebra JO

3 of 3× 3 Hermitian matricesover real octonions. Its global invariance group in 5D isE6(−26) with maximal compact subgroup F4.

I In D = 4 and D = 3 the exceptional supergravity has E7(−25)

and E8(−24) as its U-duality group while the maximal N = 8supergravity has E7(7) and E8(8), respectively.

M. Gunaydin, Istanbul,Aug. 4 2011 7

Page 12: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

N = 2 MESGTs reduce to N = 4 supersymmetric sigma modelscoupled to gravity in d = 3. The target manifolds of magicalsupergravity theories in d = 3 are the exceptional quaternionicsymmetric spaces:

IF4(4)

Usp(6)×USp(2) ,E6(2)

SU(6)×SU(2) ,E7(5)

SO(12)×SU(2) ,E8(−24)

E7×SU(2)

I The generic Jordan family of MESGT reduced to d = 3 havethe target spaces: SO(n+2,4)

SO(n+2)×SO(4)

Exceptional N = 2 versus Maximal N = 8 Supergravity:

I The exceptional N = 2 supergravity is defined by theexceptional Jordan algebra JO

3 of 3× 3 Hermitian matricesover real octonions. Its global invariance group in 5D isE6(−26) with maximal compact subgroup F4.

I In D = 4 and D = 3 the exceptional supergravity has E7(−25)

and E8(−24) as its U-duality group while the maximal N = 8supergravity has E7(7) and E8(8), respectively.

M. Gunaydin, Istanbul,Aug. 4 2011 7

Page 13: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

D = 6 D = 5 D = 4 D = 3

SO(9,1)SO(9)

−→E6(−26)

F4−→

E7(−25)

E6×SO(2)−→

E8(−24)

E7×SU(2)

SO(5,1)SO(5)

−→ SU∗(6)USp(6)

−→ SO∗(12)U(6)

−→E7(−5)

SO(12)×SU(2)

SO(3,1)SO(3)

−→ SL(3,C)SO(3)

−→ SU(3,3)SU(3)×SU(3)×U(1)

−→E6(+2)

SU(6)×SU(2)

SO(2,1)SO(2)

−→ SL(3,R)SO(3)

−→ Sp(6,R)U(3)

−→F4(+4)

USp(6)×USp(2)

Table: Scalar target spaces of magical supergravities in 6, 5, 4 and 3dimensions.

M. Gunaydin, Istanbul,Aug. 4 2011 8

Page 14: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Magical Supergravity Theories in 6 Dimensions coupled toHypermultiplets and Their Gaugings

MG, Samtleben , Sezgin , arxiv.org/1012.1818Chiral N = (1, 0) supergravity coupled to nT tensor multiplets, nV vectormultiplets and nH hypermultiplets:

supergravity and tensor multiplets : emµ , ψ

iµ,B

Iµν , χ

ai , LI ,

vector multiplets : AAµ, λ

Ai ,

hypermultiplets : φX , ψr ,

I = 0, 1, . . . , nT , a = 1, . . . , nT , A = 1, . . . , nV , X =

1, . . . , 4nH , r = 1, . . . , 2nH . The gravitino, tensorino and gaugino are all

doublets of the R-symmetry group USp(2)R (i = 1, 2). All fermions are

symplectic Majorana-Weyl, where (ψiµ, λ

Ai ) have positive chirality and

(χai , ψr ) have negative chirality. LI denotes a representative of the coset

space SO(nT , 1)/SO(nT ) parameterized by nT real scalars of tensor

multiplets.

M. Gunaydin, Istanbul,Aug. 4 2011 9

Page 15: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I nT scalars of tensor multiplets parameterize the cosetSO(nT , 1)/SO(nT ).

I Magical supergravities have nT = 2, 3, 5, 9 tensor multipletswith the vectors transforming in the spinor representation ofSO(nT , 1)

IGT Rv AA

µ ΓIAB Rten

SO(9, 1) 16c MW ΓIAB 10

SO(5, 1)× USp(2) (4c , 2) SMW, A = (αr) ΓIαr,βs = ΓIαβεrs (6, 1)

SO(3, 1)× U(1) (2, 1)+ + (1, 2)− W, A = α, β(

0 ΓIαβ

ΓIαβ 0

)(2, 2)0

SO(2, 1) 2 M ΓIAB 3

Table: GT = global symmetry groups, Rv= the representation ofvector fields under GT ; Rten =representation of tensors under GT .

I Magical supergravities satisfy

ΓI (ABΓIC)D = 0

which are the Fierz identities of supersymmetric Yang-Mills theories in thecritical dimensions 3, 4, 6, 10. Hence the Abelian gauge anomaly vanishes:

A = cεµνλρσεΓIABΓICDΛAFB

µνFCλρF

Dσε

M. Gunaydin, Istanbul,Aug. 4 2011 10

Page 16: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I nT scalars of tensor multiplets parameterize the cosetSO(nT , 1)/SO(nT ).

I Magical supergravities have nT = 2, 3, 5, 9 tensor multipletswith the vectors transforming in the spinor representation ofSO(nT , 1)

IGT Rv AA

µ ΓIAB Rten

SO(9, 1) 16c MW ΓIAB 10

SO(5, 1)× USp(2) (4c , 2) SMW, A = (αr) ΓIαr,βs = ΓIαβεrs (6, 1)

SO(3, 1)× U(1) (2, 1)+ + (1, 2)− W, A = α, β(

0 ΓIαβ

ΓIαβ 0

)(2, 2)0

SO(2, 1) 2 M ΓIAB 3

Table: GT = global symmetry groups, Rv= the representation ofvector fields under GT ; Rten =representation of tensors under GT .

I Magical supergravities satisfy

ΓI (ABΓIC)D = 0

which are the Fierz identities of supersymmetric Yang-Mills theories in thecritical dimensions 3, 4, 6, 10. Hence the Abelian gauge anomaly vanishes:

A = cεµνλρσεΓIABΓICDΛAFB

µνFCλρF

Dσε

M. Gunaydin, Istanbul,Aug. 4 2011 10

Page 17: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I nT scalars of tensor multiplets parameterize the cosetSO(nT , 1)/SO(nT ).

I Magical supergravities have nT = 2, 3, 5, 9 tensor multipletswith the vectors transforming in the spinor representation ofSO(nT , 1)

IGT Rv AA

µ ΓIAB Rten

SO(9, 1) 16c MW ΓIAB 10

SO(5, 1)× USp(2) (4c , 2) SMW, A = (αr) ΓIαr,βs = ΓIαβεrs (6, 1)

SO(3, 1)× U(1) (2, 1)+ + (1, 2)− W, A = α, β(

0 ΓIαβ

ΓIαβ 0

)(2, 2)0

SO(2, 1) 2 M ΓIAB 3

Table: GT = global symmetry groups, Rv= the representation ofvector fields under GT ; Rten =representation of tensors under GT .

I Magical supergravities satisfy

ΓI (ABΓIC)D = 0

which are the Fierz identities of supersymmetric Yang-Mills theories in thecritical dimensions 3, 4, 6, 10. Hence the Abelian gauge anomaly vanishes:

A = cεµνλρσεΓIABΓICDΛAFB

µνFCλρF

Dσε

M. Gunaydin, Istanbul,Aug. 4 2011 10

Page 18: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The bosonic field equation of the full theory including the hypermultiplets( modulo fermionic contributions):

0 = G +µνρ

0 = G a−µνρ

0 = Rµν −1

4gIJGµρσ

IGνρσJ − Pa

µPνa − 2P riµPνri

−2mAB

(FAµρFν

ρB − 1

8gµνFA

ρσF ρσB)

0 = DµPµa − 1

2ma

ABFAµνFµνB − 1

6G aµνρGµνρ

0 = DµPµri

0 = Dν

(mABFµνB

)+(mABGµνρ

− + maABGµνρ a

+

)FBνρ

G Iµνρ ≡ 3∂[µB I

νρ] + 3ΓIABFA

[µνABρ]

FAµν ≡ 2∂[µAA

ν]

Gµνρ ≡ G IµνρLI , G a

µνρ ≡ G IµνρLa

I

M. Gunaydin, Istanbul,Aug. 4 2011 11

Page 19: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The fermionic field equations ( to first order in fermionic fields)

0 = γµνρDνψiρ −

1

2Gµνργνψ

iρ −

1

2γνγµχaiPa

µ + γνγµψrPriµ

+1

2mAB

(γρσγµλAiFB

ρσ

)+

1

4Haµνργ

νρχai ,

0 = γµDµχa − 1

24γµνρχaGµνρ −

1

2ma

ABγµνλAFB

µν

+1

4G aµνργµνψρ −

1

2γµγνψµPa

ν ,

0 = γµDµψr +

1

24γµνρψrGµνρ − γµγνψµiP ri

µ ,

0 = mABγµDµλ

B +1

4maABγ

µνχaFBµν +

1

24maABγ

µνρλBG aµνρ

+1

2maABγ

µλBPaµ +

1

4mABγ

µγνρψµFBνρ ,

M. Gunaydin, Istanbul,Aug. 4 2011 12

Page 20: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The supersymmetry transformation rules ( up to cubic fermionicterms)

δemµ = εγmψµ ,

δψµ = Dµε+1

48γρστγµεGρστ ,

δcov.BµνI = −2εγ[µψν] LI + εγµνχ

a LIa ,

δχa =1

2γµεPa

µ −1

24γµνρεG a

µνρ ,

δLI = εχaLaI ,

δAAµ = εγµλ

A ,

δλA = −1

4γµνεFA

µν ,

δφX = V Xri ε

iψr ,

δψr = P riµ γ

µεi .M. Gunaydin, Istanbul,Aug. 4 2011 13

Page 21: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The field equations are derivable from the action:Ferrara, Riccioni, Sagnotti, 97 & Riccioni 2000

e−1L = R −1

12gIJG

IµνρG

µνρJ −1

4PaµP

µa −1

2PriµPµri

−1

4mABF

AµνF

µνB −1

8εµνρσλτΓIABB

IµνF

AρσF

Bλτ

+1

2ψµγ

µνρDνψρ −1

2χaγµDµχ

a −1

2ψrγµDµψr

−mAB λAγµDµλ

B +1

2ψµγνγ

µχaPνa − (ψiµγνγ

µψr )Pνri

+1

48Gµνρ

(ψλγ[λγ

µνργτ ]ψτ + χaγµνρχa − ψrγµνρψr

)+

1

24G aµνρ

(ψλγ

µνργλχa −maAB λAγµνρλB

)−

1

2FAµν

(mAB ψλγ

µνγλλB −maAB χaγµνλB

),

Note that the (anti-)selfduality conditions are imposed after the variation of the action

with respect to the 2-form potential.

M. Gunaydin, Istanbul,Aug. 4 2011 14

Page 22: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Gauging Global Symmetries of Magical Supergravity Theories in 6Dimensions via the Embedding Tensor Formalism

Dµ = ∂µ − AµA XA

XA = ΘAIJ tIJ + ΘA

X tX + ΘAAtA

the gauge group is parameterized by the embedding tensors ΘAIJ , ΘA

X ,and ΘA

A. tIJ = t[IJ] are the SO(nT , 1) generators tX generatesymmetries USp(2) and U(1) for nT = 5 and nT = 3, respectively. Thegenerators tA denote the isometries of the quaternionic Kahler manifoldof the hyperscalars. The (tIJ , tX ) generate GT and tA generate GH .Closure of the gauge algebra imposes the conditions[XA,XB ] = −X[AB]

C XC , X(AB)CXC = 0

XABC ≡ (XA)B

C evaluated in the representation Rv .

Rv = 2,4,8, 16 for the magical supergravities.

M. Gunaydin, Istanbul,Aug. 4 2011 15

Page 23: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The covariant non-abelian field strengths are

GAµν = FAµν + X(BC)

A BBCµν ,

FAµν = 2∂[µAA

ν] + X[BC ]AAB

µACν

The two-forms BABµν = B

(AB)µν transform in the symmetric tensor product

of (Rv ⊗Rv)sym, and the non-abelian gauge transformations are

δAAµ = DµΛA − X(BC)

A Λ(BC)µ ,

δBABµν = 2D[µΛAB

ν] − 2Λ(AGB)µν + 2A

(A[µδA

B)ν]

Consistency requires that the additional two-forms B(AB)µν form a subset

of the nT tensor fields in the theory and leads to the constraint

X(BC)A = ΓI

BC θAI

with a constant tensor θAI such that with the identificationB Iµν = ΓI

ABBABµν the system of gauge transformations takes the form

δΛAAµ = DµΛA − θAI ΛI

µ ,

δcov, ΛB Iµν = 2D[µΛI

ν − 2ΓIABΛAGBµν ,

whereδcov.B

Iµν = δBµν

I − 2ΓIABAA

[µδABν] ,

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Page 24: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Gauging leads to the following set of covariant field strengths

GAµν ≡ 2∂[µAAν] + X[BC ]

AABµA

Cν + B I

µνθAI ,

HIµνρ ≡ 3D[µB

Iνρ] + 6 ΓI

AB A[µA(∂νAρ]

B + 13X[CD]

BAνCAρ]

D)

+ θIA Cµνρ A ,

Gµνρσ A ≡ 4D[µCνρσ] A − (ΓI )AB

(6B I

µνGBρσ + 6θBJB I[µνBρσ]J

+ 8ΓICDA

B[µA

Cν ∂ρA

Dσ] + 2ΓI

CDXEFDA[µ

BAνCAρ

EAσ]F),

The equations of motion impose (anti-)self-duality on the dressed fieldstrengths LIGIµνρ and La

I GIµνρ and the three-form fields CµνρA are on-shelldual to the vector fields:

e θAI GµνρλA = −1

2εµνρλστ mAB GAστθBI ,

mAB ≡ LIΓIAB , ma

AB ≡ LaI ΓI

AB

M. Gunaydin, Istanbul,Aug. 4 2011 17

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Closure of the gauge algebra on the two-form fields require:

(XA)IJ = 2

(θBI ΓJ

AB − θJB(ΓI )AB)⇒ ΘA

IJ = −Γ[IAB θ

J]B

Recall XA = ΘAIJ tIJ + ΘA

X tX + ΘAAtA The constraints imply that

θIA = ζAξI where ζA is an unconstrained (commuting) spinor ofSO(nT , 1) , ξI ξI = 0 and the unique solution

ξI = ΓIABζ

AζB

The magical Fierz identities imply that ξI is null and ΓIABθ

BI = 0.

The gauging is uniquely determined by the choice of a constant

commuting spinor ζA of SO(nT , 1). Spinors belonging to different orbits

describe inequivalent gaugings ⇒ Hence the classification of possible

gaugings is equivalent to classification of inequivalent orbits of the spinor

representation of SO(nT , 1).

M. Gunaydin, Istanbul,Aug. 4 2011 18

Page 26: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Spinor OrbitsRecall that in 5d magical MESGTs are defined by simple Jordan algebras of degreethree with isometry groups SL(3,R), SL(3,C), SU∗(6),E6(−26)

Str0[R⊕ JR2 ] = SO(1, 1)× Spin (2, 1) ⊂ SL (3,R)

Str0[R⊕ JC2 ] = SO(1, 1)× Spin (3, 1) ⊂ SL (3,C)

Str0[R⊕ JH2 ] = SO(1, 1)× Spin (5, 1) ⊂ SU∗ (6)

Str0[R⊕ JO2 ] = SO(1, 1)× Spin (9, 1) ⊂ E6(−26)

A general element X ∈ JA3 decomposes w.r.t Jordan subalgebra JA2 as

X =

(JA2 ψ(A)

ψ†(A) R

); ψ(A) =

(q1

q2

)

JA2 ⇐⇒ tensor fields in 6d

ψ†(A) ⇐⇒ vector fields in 6d ⇐⇒ Spinors of SO(nT , 1)

M. Gunaydin, Istanbul,Aug. 4 2011 19

Page 27: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Orbits of ψ(A) under the action of SO(nT , 1) = Str0(JA2 )Bryant

Str0(JR2 ) = Spin(2, 1) = SL(2,R)

Str0(JC2 ) = Spin(3, 1) = SL(2,C)

Str0(JH2 ) = Spin(5, 1) = SL(2,H)

Str0(JO2 ) = Spin(9, 1) = SL(2,O)

There exists a unique nontrivial orbit for all the magical theories consisting of theentire spinor space;

Orbit(ψ(O)) =Spin(9, 1)

Spin(7)sT8

where T8 denotes the eight dimensional translations.

Orbit(ψ(H)) =Spin(5, 1)

SU(2)sT4

Complex two component spinor ψ(C) is a Weyl spinor and forms a single orbit ofSL(2,C) = Spin(3, 1)

Orbit(ψ(C)) =SL(2,C)

T2

Restricting to real spinors one finds

Orbit(ψ(R)) =SL(2,R)

T1

M. Gunaydin, Istanbul,Aug. 4 2011 20

Page 28: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The gauge group generators in the vector/tensor sector in terms of thespinor ζA:

(XA)BC =(ζΓI ζ)(ΓJζ)A(ΓIJ)B

C ; (XA)IJ =4 (ζΓ[I ζ)(ΓJ]ζ)A

They satisfy

(XAXB)CD = 0 ; (XAXB XC )I

J = 0 ,

They span an (nT − 1)-dimensional nilpotent abelian algebra and gauge(nT − 1) translations.This is the unique possible gauge group and furthermore the (nT − 1)translations can not lie strictly within the isometry group SO(nT , 1) dueto the appearance of central extensions of the gauge algebra!For the octonionic magical theory nT = 9 the compact part of thestability (little) group of a Majorana-Weyl spinor (16) of SO(9, 1) isSpin(7) under which we have

ζA : 16c → 8+ + 7− + 1− , ξI : 10 → 80 + 1+2 + 1−2

A→ (α, t, 0) , I → (α,+,−) ,

corresponding to the choice ζA = 12 (~0,~0, g 1/3).

M. Gunaydin, Istanbul,Aug. 4 2011 21

Page 29: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

In this basis, the gauge algebra becomes:

[Xα,Xβ ] = −gγtαβ Xt [Xα,Xt ] = 0 = [Xt ,Xu ] , X0 = 0 .

The generators Xt act as central extensions of the algebra that vanish when acting onvector or tensor fields. They may act non-trivially in the hypermultiplet sector.Consider its embedding in the U-duality group of the corresponding 5d MESGT:

E6(−26) = K16c ⊕ SO(9, 1)× SO(1, 1)D ⊕ T16c

where T16c are the 16 translational symmetries corresponding to Abelian gaugesymmetries of 16 vector fields of 6D theory. SO(9, 1) admits a three grading withrespect to its SO(8)× SO(1, 1)∆. Thus E6(−26) has the 5× 3 grading w.r.tSO(8)× SO(1, 1)D × SO(1, 1)∆ subgroup:

T8c T8s

N8v −−−− (SO(8)× SO(1, 1)∆ × SO(1, 1)D) −−−− N8v

K8s K8c

Table:

M. Gunaydin, Istanbul,Aug. 4 2011 22

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T8 = Tα T1 + T7 = Tt

N8 −− (Spin(7) + 7)× SO(1, 1)2 −− N8 = Nα

K7+1 K8

Table: 5× 3 decomposition of E6(−26) with respect to Spin(7).Xα = (Tα + Nα)⊕ Xt = Tt generate a centrally extended nilpotentAbelian subgroup of E6(−26)

The nilpotent Abelian group generated by Xα with central elements Tt

can be embedded in the F4(−20) subgroup of E6(−26) as follows:

F4(−20) = 7−2 ⊕ 8−1 ⊕ Spin(7)× SO(1, 1)⊕ 8+1 ⊕ 7+2

where (Xα ⊕ Tt) ≡ (8+1 ⊕ 7+2)M. Gunaydin, Istanbul,Aug. 4 2011 23

Page 31: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

Embedding of nilpotent Abelian gauge grous with central charges:

E6(−26) ⊃ F4(−20) = 7−2 ⊕ 8−1 ⊕ Spin(7)× SO(1, 1)⊕ 8+1 ⊕ 7+2

SU∗(6) ⊃ USp(4, 2) = 3−2 ⊕ 4−1 ⊕ SU(2)× SO(1, 1)⊕ 4+1 ⊕ 3+2

SL(3,C) ⊃ SU(2, 1) = 1−2 ⊕ 2−1 ⊕ U(1)× SO(1, 1)⊕ 2+1 ⊕ 1+2

SL(3,R) ⊃ SL(2,R) = 1−1 ⊕ SO(1, 1)⊕ 1+1

Gauging in the Hypersector:To gauge isometries of the quaternionic Kahler manifold that couples tomagical sugras , consider the full generator XA = ΘA

IJ tIJ + ΘAAtA in

the embedding tensor formalism with non-vanishing ΘAA ( tA). The

generators of isometries are tA which act on the quaternionic Kahler viaKilling vector fields KX

A = tA · φX .

[XA,XB ] = −X[AB]C XC , X(AB)

CXC = 0

M. Gunaydin, Istanbul,Aug. 4 2011 24

Page 32: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The gauging in the hypersector of the octonionic magical supergravitycorresponds to selecting 8+7 Killing vector fields Kα ≡ Θα

AKA,Kt ≡ Θt

AKA (not necessarily linearly independent), which satisfy thealgebra

[Kα,Kβ] = −gγtαβ Kt , [Kα,Kt ] = 0 = [Kt ,Ku]

Thus, the generators associated with the full gauge group in the magicalsupergravities, including both the vector-tensor and hyper sectors, are

XA = Xα +Kα ,Kt ,

In contrast to the vector/tensor sector, in the hypersector the generatorsKt may act as nontrivial central charges of the gauge algebra. thenilpotent gauge algebra of the octonionic magical theory with all sevenKt non-vanishing can be embedded into the Lie algebra of the groupF4(−20) which admits the five grading

7−2 ⊕ 8−1 ⊕ Spin(7)0 ⊕ SO(1, 1)0 ⊕ 8+1 ⊕ 7+2

with the generators of positive grading corresponding to the nilpotentgauge group. The group F4(−20) may be embedded into the isometrygroup of the hypermatter described by the quaternionic Kahler manifoldE8(−24)/(E7 × SU(2)) such that all 7 central ”charges” act nontrivially onthe hypersector when the octonionic magical theory is coupled to it.

M. Gunaydin, Istanbul,Aug. 4 2011 25

Page 33: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The octonionic magical theory coupled to hypermultiplets belonging toE8(−24)/E7 × SU(2) is free of gravitational anomalies in six dimensions and reduces toa double exceptional theory in 3d with the scalar manifold MG & Sezgin

M3 = [E8(−24)

(E7 × SU(2))]× [

E8(−24)

(E7 × SU(2))]

The moduli space of the FSHV model with the is a subsector of this theory.The nilpotent gauge algebra of the quaternionic magical theory can be embedded intothe Lie algebra of USp(4, 2) which is quaternionic real. The quaternionic symmetricspace of minimal dimension whose isometry group includes the nilpotent gauge groupwith all three central charges is

USp(4, 2)

USp(4)× USp(2)

Gauge group can also be embedded in

E7(−5)

SO(12)× SU(2)

The scalar manifold of the ungauged quaternionic magical theory coupled to thishypermatter has the double exceptional isometry group in three dimensions:

E7(−5)

SO(12)× SU(2)×

E7(−5)

SO(12)× SU(2)

For the complex magical theory the nilpotent gauge group embeds into SU(2, 1)which is quaternionic real. Thus the minimal hypermanifold in this case is

SU(2, 1)

U(2)

we can also couple the theory to hypermultiplets with the target manifold

E6(2)

SU(6)× SU(2)

Again the corresponding 3D target space with this hypersector is doubly exceptional.

M. Gunaydin, Istanbul,Aug. 4 2011 26

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M/Superstring Theoretic Origins of N = 2 MESGTs withSymmetric Scalar ManifoldsQuaternionic magical 4d MESGT without any hypermultiplets can be obtained fromIIB superstring by compactifications of type IIB on an orbifold of T 4 × S1 × S1.

Sen, Vafa (1995) & MG 2006The 6d octonionic magical MESGT coupled to 28 hypermultiplets parametrizing thequaternionic symmetric space E8(−24)/E7 × SU(2) is free of gravitational anomalies.(nH − nV + 29nT = 273). Its 4d scalar manifold contains the moduli space of FHSVmodel which is obtained from IIB superstring by compactification on a self-mirrorCalabi-Yau manifold with Hodge numbers h(1,1) = h(2,1) = 11 :

MV ×MH =E7(−25)

E6 × U(1)×

E8(−24)

E7 × SU(2)⊃

SO(10, 2)× SU(1, 1)

SO(10)× U(1)× U(1)×

SO(12, 4)

SO(12)× SO(4)

Bianchi and Ferrara (2008) reconsidered the string derivation of FSHV model over theEnriques Calabi-Yau and argued that the octonionic magical MESGT admits a stringinterpretation closely related to the Enriques model.Type IIB superstring theory compactified over a CY threefold constructed by Todorovleads to the complex magical N = 2 MESGT in d = 4 coupled to (h(1,1) + 1) = 30hypermultiplets.

The hyper-free N = 2 string models based on asymmetric orbifolds with N = (4, 1)

world-sheet superconformal symmetry using 2D fermionic construction given by

Dolivet, Julia and Kounnas include the complex and quaternionic magical

supergravities in d = 4.

M. Gunaydin, Istanbul,Aug. 4 2011 27

Page 35: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

U-duality Orbits of Extremal , Spherically Symmetric StationaryBlack Hole Solutions of 5D Supergravity Theories with SymmetricTarget Spaces: ( MG and Ferrara, 1997 )

I The black hole potential that determines the attractor flowtakes on the following form for N = 2 MESGTs: (Ferrara, Gibbons,

Kallosh, Strominger )

V (φ, q) = qIaIJ

qJ

whereaIJ is the ”metric” of the kinetic energy term of the

vector fields. The (n + 1) dimensional charge vector in anextremal BH background is given by

qI =

∫S3

HI =

∫S3

aIJ ∗F J (I = 0, 1, ...n)

The entropy S of an extremal black hole solution of N = 2MESGT with charges qI is determined by the value of theblack hole potential V at the attractor points

SBPS = (Vcritical)3/4 =

(C IJKqIqJqK

)3/4

M. Gunaydin, Istanbul,Aug. 4 2011 28

Page 36: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

J OBPS = Str0(J)/Aut(J)JR

3 SL(3,R)/SO(3)JC

3 SL(3,C)/SU(3)JH

3 SU∗(6)/USp(6)

JO3 E6(−26)/F4

R⊕ Γ(1,n−1) SO(n − 1, 1)× SO(1, 1)/SO(n − 1)

Table: Orbits of spherically symmetric stationary BPS black holesolutions in 5D MESGTs defined by Euclidean Jordan algebras J ofdegree three. U-duality and stability groups are given by the Lorentz (reduced structure ) and rotation ( automorphism) groups of J.

J Onon−BPS = Str0(J)/Aut(J(1,2))JR

3 SL(3,R)/SO(2, 1)JC

3 SL(3,C)/SU(2, 1)JH

3 SU∗(6)/USp(4, 2)

JO3 E6(−26)/F4(−20)

R⊕ Γ(1,n−1) SO(n − 1, 1)× SO(1, 1)/SO(n − 2, 1)

Table: Orbits of non-BPS extremal BHs with non-zero entropy.

M. Gunaydin, Istanbul,Aug. 4 2011 29

Page 37: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

The orbits of BPS black hole solutions of N = 8supergravity theory in five dimensions.

The 1/8 BPS black holes with non-vanishing entropy has the orbit

O1/8−BPS =E6(6)

F4(4)

Maximal supergravity theory admits 1/4 and 1/2 BPS black holesolutions with vanishing entropy. Their orbits under U-duality are

O1/4−BPS =E6(6)

O(5, 4)sT16

O1/2−BPS =E6(6)

O(5, 5)sT16

Vanishing entropy means vanishing cubic norm. Thus the black holesolutions corresponding to vanishing entropy has additional symmetriesbeyond the five dimensional U-duality group.

=⇒ They are invariant under the generalized special conformal

transformations of the underlying Jordan algebras.M. Gunaydin, Istanbul,Aug. 4 2011 30

Page 38: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I The proposal that the conformal groups Conf [J] of underlyingJordan algebras J of supergravity theories must act asspectrum generating symmetry groups.Conf [J] leaves invariant light-like separations with respect toa cubic distance function N3(J1 − J2) and has a natural3-grading with respect to their Lorentz subgroups

Conf [J] = KJ ⊕ Lor(J)×D ⊕ TJ

Lor(J) is the 5D U-duality group that leaves the cubic norminvariant.

I Conf [J]⇔ U-duality group of corresponding 4D supergravity.

I 4D U-duality groups must act as spectrum generatingsymmetry groups of corresponding five dimensionalsupergravity theories.

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Page 39: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I The proposal that the conformal groups Conf [J] of underlyingJordan algebras J of supergravity theories must act asspectrum generating symmetry groups.Conf [J] leaves invariant light-like separations with respect toa cubic distance function N3(J1 − J2) and has a natural3-grading with respect to their Lorentz subgroups

Conf [J] = KJ ⊕ Lor(J)×D ⊕ TJ

Lor(J) is the 5D U-duality group that leaves the cubic norminvariant.

I Conf [J]⇔ U-duality group of corresponding 4D supergravity.

I 4D U-duality groups must act as spectrum generatingsymmetry groups of corresponding five dimensionalsupergravity theories.

M. Gunaydin, Istanbul,Aug. 4 2011 31

Page 40: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I The proposal that the conformal groups Conf [J] of underlyingJordan algebras J of supergravity theories must act asspectrum generating symmetry groups.Conf [J] leaves invariant light-like separations with respect toa cubic distance function N3(J1 − J2) and has a natural3-grading with respect to their Lorentz subgroups

Conf [J] = KJ ⊕ Lor(J)×D ⊕ TJ

Lor(J) is the 5D U-duality group that leaves the cubic norminvariant.

I Conf [J]⇔ U-duality group of corresponding 4D supergravity.

I 4D U-duality groups must act as spectrum generatingsymmetry groups of corresponding five dimensionalsupergravity theories.

M. Gunaydin, Istanbul,Aug. 4 2011 31

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I Under dimensional reduction of 5D MESGT to 4D

M5 =Lor(J)

Rot(J)⇒ M4 =

Conf (J)

Lor(J)× U(1)

where Lor(J) is the compact real form of the Lorentz group ofJ. The bosonic sector of dimensionally reduced Lagrangian is

e−1L(4) = −1

2R − gI J(∂µz I )(∂µzJ)

+1

4Im(NAB)FA

µνFµνB − 1

8Re(NAB)εµνρσFA

µνFBρσ

In 5D: Vector fields AµI ⇔ Elements of Jordan algebra J

In 4D: FAµν ⊕ FA

µν ⇔ Elements of a Freudenthal triple system(FTS) F(J) :

X =

R J F 0µν F I

µν

⇔J R F I

µν F 0µν

M. Gunaydin, Istanbul,Aug. 4 2011 32

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I U-duality group G4 of a 4D Maxwell-Einstein supergravity ⇔Aut(F(J)) ≡ Conf [J]

I The entropy of an extremal dyonic black hole with charges(p0, pI , q0, qI ) is given by the quartic invariant Q4(q, p) of theFreudenthal triple system F(J).

I black hole attractor equations ⇒ criticality conditions forblack hole scalar potential

VBH ≡ |Z |2 + G I J(DIZ )(DJZ )

Z ≡ central charge function.

I

∂IVBH = 0

implies

2Z DIZ + iCIJKG JJGKKDJZ DKZ = 0

M. Gunaydin, Istanbul,Aug. 4 2011 33

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J

12

-BPS orbitsO 1

2−BPS

non-BPS, Z 6= 0 orbitsOnon−BPS,Z 6=0

non-BPS, Z = 0 orbitsOnon−BPS,Z=0

− SU(1,n+1)SU(n+1)

− SU(1,n+1)SU(1,n)

R⊕ Γ(1,n−1)SU(1,1)⊗SO(2,2+n)SO(2)⊗SO(2+n)

SU(1,1)⊗SO(2,2+n)SO(1,1)⊗SO(1,1+n)

SU(1,1)⊗SO(2,2+n)SO(2)⊗SO(2,n)

JO3E7(−25)

E6

E7(−25)E6(−26)

E7(−25)E6(−14)

JH3SO∗(12)SU(6)

SO∗(12)SU∗(6)

SO∗(12)SU(4,2)

JC3SU(3,3)

SU(3)⊗SU(3)SU(3,3)SL(3,C)

SU(3,3)SU(2,1)⊗SU(1,2)

JR3Sp(6,R)SU(3)

Sp(6,R)SL(3,R)

Sp(6,R)SU(2,1)

Table: Non-degenerate orbits of N = 2, D = 4 MESGTs with symmetricscalar manifolds. Except for the first row all such theories originate fromfive dimensions and are defined by Jordan algebras that are indicated inthe first column. Bellucci, Ferrara , MG, Marrani

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I The orbits of BH solutions of 4D N = 8 supergravity underE7(7):

I4 > 0 : O 18−BPS =

E7(7)

E6(2)⇐⇒ 1

8-BPS;

I4 < 0 : Onon−BPS =E7(7)

E6(6)⇐⇒ non-BPS.

Generic light-like orbit with 1 vanishing eigenvalue:

E7(7)

F4(4)sT26

Critical light-like orbit with 2 vanishing eigenvalues:

E7(7)

O(6, 5)s(T32 ⊕ T1)

Doubly critical light-like orbit with 3 vanishing eigenvalues :

E7(7)

E6(6)sT27

M. Gunaydin, Istanbul,Aug. 4 2011 35

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I Classification of the orbits of spherically symmetric stationaryextremal black holes of 4D, N = 8 sugra and 4D, N = 2MESGTs with symmetric target spaces. ( Ferrara and MG , 1997 ).

I Question: Can the 3D U-duality groups act as spectrumgenerating conformal symmetries of corresponding 4Dsupergravity theories ? ( MG, Koepsell, Nicolai )

I No conformal realization for any real forms of E8,G2 and F4

⇔ No 3-grading with respect to a subgroup of maximal rank.

I However, all simple Lie algebras admit a 5-grading withrespect to a subalgebra of maximal rank

g = g−2 ⊕ g−1 ⊕ g0 ⊕ g+1 ⊕ g+2

such that the grade ±2 subspaces are one-dimensional.

M. Gunaydin, Istanbul,Aug. 4 2011 36

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I Classification of the orbits of spherically symmetric stationaryextremal black holes of 4D, N = 8 sugra and 4D, N = 2MESGTs with symmetric target spaces. ( Ferrara and MG , 1997 ).

I Question: Can the 3D U-duality groups act as spectrumgenerating conformal symmetries of corresponding 4Dsupergravity theories ? ( MG, Koepsell, Nicolai )

I No conformal realization for any real forms of E8,G2 and F4

⇔ No 3-grading with respect to a subgroup of maximal rank.

I However, all simple Lie algebras admit a 5-grading withrespect to a subalgebra of maximal rank

g = g−2 ⊕ g−1 ⊕ g0 ⊕ g+1 ⊕ g+2

such that the grade ±2 subspaces are one-dimensional.

M. Gunaydin, Istanbul,Aug. 4 2011 36

Page 47: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Classification of the orbits of spherically symmetric stationaryextremal black holes of 4D, N = 8 sugra and 4D, N = 2MESGTs with symmetric target spaces. ( Ferrara and MG , 1997 ).

I Question: Can the 3D U-duality groups act as spectrumgenerating conformal symmetries of corresponding 4Dsupergravity theories ? ( MG, Koepsell, Nicolai )

I No conformal realization for any real forms of E8,G2 and F4

⇔ No 3-grading with respect to a subgroup of maximal rank.

I However, all simple Lie algebras admit a 5-grading withrespect to a subalgebra of maximal rank

g = g−2 ⊕ g−1 ⊕ g0 ⊕ g+1 ⊕ g+2

such that the grade ±2 subspaces are one-dimensional.

M. Gunaydin, Istanbul,Aug. 4 2011 36

Page 48: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Classification of the orbits of spherically symmetric stationaryextremal black holes of 4D, N = 8 sugra and 4D, N = 2MESGTs with symmetric target spaces. ( Ferrara and MG , 1997 ).

I Question: Can the 3D U-duality groups act as spectrumgenerating conformal symmetries of corresponding 4Dsupergravity theories ? ( MG, Koepsell, Nicolai )

I No conformal realization for any real forms of E8,G2 and F4

⇔ No 3-grading with respect to a subgroup of maximal rank.

I However, all simple Lie algebras admit a 5-grading withrespect to a subalgebra of maximal rank

g = g−2 ⊕ g−1 ⊕ g0 ⊕ g+1 ⊕ g+2

such that the grade ±2 subspaces are one-dimensional.

M. Gunaydin, Istanbul,Aug. 4 2011 36

Page 49: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I QUASICONFORMAL REALIZATION OF E8(8) OVERA 57 DIMENSIONAL SPACE MG, Koepsell, Nicolai

E8(8) = 1−2 ⊕ 56−1 ⊕ E7(7) + SO(1, 1)⊕ 56+1 ⊕ 1+2

g = K ⊕ UA ⊕ [S(AB) + ∆]⊕ UA ⊕ K

over a space T coordinatized by the elements X of FTS Fplus an extra singlet variable x : 56+1 ⊕ 1+2 ⇔ (X , x) ∈ T :

K (X ) = 0

K (x) = 2

UA (X ) = A

UA (x) = 〈A,X 〉SAB (X ) = (A,B,X )

SAB (x) = 2 〈A,B〉 x

UA (X ) =1

2(X ,A,X )− Ax

UA (x) = −1

6〈(X ,X ,X ) ,A〉+ 〈X ,A〉 x

K (X ) = −1

6(X ,X ,X ) + Xx

K (x) =1

6〈(X ,X ,X ) ,X 〉+ 2 x2

Freudenthal triple product ⇔ (X ,Y ,Z )skew-symmetric invariant form ⇔ 〈X ,Y 〉 = −〈Y ,X 〉

M. Gunaydin, Istanbul,Aug. 4 2011 37

Page 50: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Geometric meaning of the quasiconformal action of the Liealgebra g on the space T ?

I Define a quartic norm of X = (X , x) ∈ T asN4(X ) := Q4(X )− x2

Q4(X ) is the quartic norm of X ∈ F .I Define a quartic “distance” function between any two pointsX = (X , x) and Y = (Y , y) in T as

d(X ,Y) := N4(δ(X ,Y)

δ(X ,Y) is the “symplectic” difference of X and Y :

δ(X ,Y) := (X − Y , x − y + 〈X ,Y 〉) = −δ(Y,X )

I Light-like separations d(X ,Y) = 0 are left invariant underquasiconformal group action.−→ Quasiconformal groups are the invariance groups of”light-cones” defined by a quartic distance function.

I E8(8) is the invariance group of a quartic light-cone in 57dimensions!

M. Gunaydin, Istanbul,Aug. 4 2011 38

Page 51: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Geometric meaning of the quasiconformal action of the Liealgebra g on the space T ?

I Define a quartic norm of X = (X , x) ∈ T asN4(X ) := Q4(X )− x2

Q4(X ) is the quartic norm of X ∈ F .

I Define a quartic “distance” function between any two pointsX = (X , x) and Y = (Y , y) in T as

d(X ,Y) := N4(δ(X ,Y)

δ(X ,Y) is the “symplectic” difference of X and Y :

δ(X ,Y) := (X − Y , x − y + 〈X ,Y 〉) = −δ(Y,X )

I Light-like separations d(X ,Y) = 0 are left invariant underquasiconformal group action.−→ Quasiconformal groups are the invariance groups of”light-cones” defined by a quartic distance function.

I E8(8) is the invariance group of a quartic light-cone in 57dimensions!

M. Gunaydin, Istanbul,Aug. 4 2011 38

Page 52: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Geometric meaning of the quasiconformal action of the Liealgebra g on the space T ?

I Define a quartic norm of X = (X , x) ∈ T asN4(X ) := Q4(X )− x2

Q4(X ) is the quartic norm of X ∈ F .I Define a quartic “distance” function between any two pointsX = (X , x) and Y = (Y , y) in T as

d(X ,Y) := N4(δ(X ,Y)

δ(X ,Y) is the “symplectic” difference of X and Y :

δ(X ,Y) := (X − Y , x − y + 〈X ,Y 〉) = −δ(Y,X )

I Light-like separations d(X ,Y) = 0 are left invariant underquasiconformal group action.−→ Quasiconformal groups are the invariance groups of”light-cones” defined by a quartic distance function.

I E8(8) is the invariance group of a quartic light-cone in 57dimensions!

M. Gunaydin, Istanbul,Aug. 4 2011 38

Page 53: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Geometric meaning of the quasiconformal action of the Liealgebra g on the space T ?

I Define a quartic norm of X = (X , x) ∈ T asN4(X ) := Q4(X )− x2

Q4(X ) is the quartic norm of X ∈ F .I Define a quartic “distance” function between any two pointsX = (X , x) and Y = (Y , y) in T as

d(X ,Y) := N4(δ(X ,Y)

δ(X ,Y) is the “symplectic” difference of X and Y :

δ(X ,Y) := (X − Y , x − y + 〈X ,Y 〉) = −δ(Y,X )

I Light-like separations d(X ,Y) = 0 are left invariant underquasiconformal group action.−→ Quasiconformal groups are the invariance groups of”light-cones” defined by a quartic distance function.

I E8(8) is the invariance group of a quartic light-cone in 57dimensions!

M. Gunaydin, Istanbul,Aug. 4 2011 38

Page 54: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Scalar manifolds of N = 2 MESGTs defined by Jordanalgebras of degree three ( 8 real supersymmetries)

M5 =Lor(J)

Rot(J)

M4 =Conf (J)

Lor(J)× U(1)

M3 =QConf (J)

Conf (J)× SU(2)I Quasiconformal extensions of 4D U-duality groups ≡ 3D

U-duality groups.I Extremal black hole solution of 4D , N = 8 sugra with 56

charges qI , pI and entropy s: light-like vectors in 57

dimensional charge-entropy space

N4(qI , pI , s) = 0→ Q4 = s2

I Proposal: 3D U-duality groups must act as spectrumgenerating symmetry groups of the extremal black holesolutions of 4D supergravity theories. GKN 2000

M. Gunaydin, Istanbul,Aug. 4 2011 39

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M5 = M4 = M3 =

J Lor (J) /Rot (J) Conf (J) / Lor (J)× U(1) QConf(F(J))/ ˜Conf (J)× SU(2)

JR3 SL(3,R)/SO(3) Sp(6,R)/U(3) F4(4)/USp(6)× SU(2)

JC3 SL(3,C)/SU(3) SU(3, 3)/S (U(3)× U(3)) E6(2)/SU(6)× SU(2)

JH3 SU∗(6)/USp(6) SO∗(12)/U(6) E7(−5)/SO(12)× SU(2)

JO3 E6(−26)/F4 E7(−25)/E6 × U(1) E8(−24)/E7 × SU(2)

R⊕ Γ(1,n−1)SO(n−1,1)×SO(1,1)

SO(n−1)SO(n,2)×SU(1,1)

SO(n)×SO(2)×U(1)SO(n+2,4)

SO(n+2)×SO(4)

Table: Scalar manifolds Md of N = 2 MESGT’s defined by Jordan

algebras J of degree 3 in d = 3, 4, 5 dimensions. Lor (J) and Conf (J)denote the compact real forms of the Lorentz group Lor (J) andconformal group Conf (J) of a Jordan algebra J. QConf (F (J)) denotesthe quasiconformal group associated with J.

M. Gunaydin, Istanbul,Aug. 4 2011 40

Page 56: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I A concrete implementation of the proposal that 3D U-dualitygroups must act as spectrum generating quasiconformalgroups of spherically symmetric stationary BPS black holes of4D supergravity theories:

MG, Neitzke, Pavlyk, Pioline, Waldrom 2005,2006

I Equations of motion for a spherically symmetric stationaryblack hole of four dimensional supergravity theories areequivalent to equations for geodesic motion of a fiducialparticle on the moduli space M∗3 of 3D supergravity obtainedby reduction on a time-like circle.

Breitenlohner, Gibbons, Maison 1987

I 3D scalar manifold from compactification on a space-like circle

M3 =G3

K3

where K3 is the maximal compact subgroup of G3.On a time-like circle one gets the scalar manifold

M∗3 =G3

H3

where H3 is a noncompact real form of K3.

M. Gunaydin, Istanbul,Aug. 4 2011 41

Page 57: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I A concrete implementation of the proposal that 3D U-dualitygroups must act as spectrum generating quasiconformalgroups of spherically symmetric stationary BPS black holes of4D supergravity theories:

MG, Neitzke, Pavlyk, Pioline, Waldrom 2005,2006

I Equations of motion for a spherically symmetric stationaryblack hole of four dimensional supergravity theories areequivalent to equations for geodesic motion of a fiducialparticle on the moduli space M∗3 of 3D supergravity obtainedby reduction on a time-like circle.

Breitenlohner, Gibbons, Maison 1987

I 3D scalar manifold from compactification on a space-like circle

M3 =G3

K3

where K3 is the maximal compact subgroup of G3.On a time-like circle one gets the scalar manifold

M∗3 =G3

H3

where H3 is a noncompact real form of K3.M. Gunaydin, Istanbul,Aug. 4 2011 41

Page 58: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

nQ nV M4 M∗3 J

8 1 ∅ U(2,1)U(1,1)×U(1) R

8 2 SL(2,R)U(1)

G2,2

SO(2,2) R8 7 Sp(6,R)

SU(3)×U(1)

F4(4)

Sp(6,R)×SL(2,R) JR3

8 10 SU(3,3)SU(3)×SU(3)×U(1)

E6(2)

SU(3,3)×SL(2,R) JC3

8 16 SO∗(12)SU(6)×U(1)

E7(−5)

SO∗(12)×SL(2,R) JH3

8 28E7(−25)

E6×U(1)

E8(−24)

E7(−25)×SL(2,R) JO3

8 n + 2 SL(2,R)U(1) ×

SO(n,2)SO(n)×SO(2)

SO(n+2,4)SO(n,2)×SO(2,2) R⊕ Γ(1,n−1)

16 n + 2 SL(2,R)U(1) ×

SO(n−4,6)SO(n−4)×SO(6)

SO(n−2,8)SO(n−4,2)×SO(2,6) R⊕ Γ(5,n−5)

24 16 SO∗(12)SU(6)×U(1)

E7(−5)

SO∗(12)×SL(2,R ) JH3

32 28E7(7)

SU(8)

E8(8)

SO∗(16) JOs

3

Table: Above we give the number of supercharges nQ , 4D vector fieldsnV , scalar manifolds of supergravity theories before and after reductionalong a timelike Killing vector from D = 4 to D = 3, and associatedJordan algebras J. Isometry groups of 4D and 3D supergravity theoriesare given by Conf (J) and QConf (J), of J, respectively.

M. Gunaydin, Istanbul,Aug. 4 2011 42

Page 59: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I The quantization of the motion of fiducial particle on M∗3leads to quantum mechanical wave functions that provide thebasis of a unitary representation of the isometry group G3 ofM∗3 .

I BPS black holes correspond to a special class of geodesicswhich lift holomorphically to the twistor space Z3 of M∗3.Spherically symmetric stationary BPS black holes of N = 2MESGT’s are described by holomorphic curves in Z3

I The relevant unitary representations of the 3D isometrygroups QConf (J) for BPS black holes are those induced bytheir holomorphic actions on the corresponding twistor spacesZ3, which belong to quaternionic discrete seriesrepresentations.

I For rank two quaternionic groups SU(2, 1) and G2(2) unitaryrepresentations induced by the geometric quasiconformalactions and their spherical vectors were studied in MG, Neitzke, Pavlyk

, Pioline (2007).

M. Gunaydin, Istanbul,Aug. 4 2011 43

Page 60: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I The quantization of the motion of fiducial particle on M∗3leads to quantum mechanical wave functions that provide thebasis of a unitary representation of the isometry group G3 ofM∗3 .

I BPS black holes correspond to a special class of geodesicswhich lift holomorphically to the twistor space Z3 of M∗3.Spherically symmetric stationary BPS black holes of N = 2MESGT’s are described by holomorphic curves in Z3

I The relevant unitary representations of the 3D isometrygroups QConf (J) for BPS black holes are those induced bytheir holomorphic actions on the corresponding twistor spacesZ3, which belong to quaternionic discrete seriesrepresentations.

I For rank two quaternionic groups SU(2, 1) and G2(2) unitaryrepresentations induced by the geometric quasiconformalactions and their spherical vectors were studied in MG, Neitzke, Pavlyk

, Pioline (2007).

M. Gunaydin, Istanbul,Aug. 4 2011 43

Page 61: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Unified realization of 3D U-duality groups of all N = 2MESGTs defined by Jordan algebras as spectrum generatingquasiconformal groups covariant with respect to their 5DU-duality groups. MG, Pavlyk (2009)

I The spherical vectors of quasiconformal realizations ofF4(4),E6(2),E7(−5),E8(−24) and SO(d + 2, 4) twisted by aunitary character ν with respect to their maximal compactsubgroups as well as their quadratic Casimir operators

I Unified realization of F4(4),E6(6),E7(7),E8(8) and ofSO(n + 3,m + 3) as QCGs covariant with respect toSL(3,R),SL(3,R)× SL(3,R),SL(6,R),E6(6) andSO(n,m)× SO(1, 1), respectively, their spherical vectors andquadratic Casimir operators.

I For ν = −(nV + 2) + iρ the quasiconformal action inducesunitary representations that belong to the principle series. Forspecial discrete values of ν the quasiconformal action leads tounitary representations belonging to the discrete series andtheir continuations. For the quaternionic real forms theybelong to the quaternionic discrete series.

M. Gunaydin, Istanbul,Aug. 4 2011 44

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I Unified realization of 3D U-duality groups of all N = 2MESGTs defined by Jordan algebras as spectrum generatingquasiconformal groups covariant with respect to their 5DU-duality groups. MG, Pavlyk (2009)

I The spherical vectors of quasiconformal realizations ofF4(4),E6(2),E7(−5),E8(−24) and SO(d + 2, 4) twisted by aunitary character ν with respect to their maximal compactsubgroups as well as their quadratic Casimir operators

I Unified realization of F4(4),E6(6),E7(7),E8(8) and ofSO(n + 3,m + 3) as QCGs covariant with respect toSL(3,R),SL(3,R)× SL(3,R),SL(6,R),E6(6) andSO(n,m)× SO(1, 1), respectively, their spherical vectors andquadratic Casimir operators.

I For ν = −(nV + 2) + iρ the quasiconformal action inducesunitary representations that belong to the principle series. Forspecial discrete values of ν the quasiconformal action leads tounitary representations belonging to the discrete series andtheir continuations. For the quaternionic real forms theybelong to the quaternionic discrete series.

M. Gunaydin, Istanbul,Aug. 4 2011 44

Page 63: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I Unified realization of 3D U-duality groups of all N = 2MESGTs defined by Jordan algebras as spectrum generatingquasiconformal groups covariant with respect to their 5DU-duality groups. MG, Pavlyk (2009)

I The spherical vectors of quasiconformal realizations ofF4(4),E6(2),E7(−5),E8(−24) and SO(d + 2, 4) twisted by aunitary character ν with respect to their maximal compactsubgroups as well as their quadratic Casimir operators

I Unified realization of F4(4),E6(6),E7(7),E8(8) and ofSO(n + 3,m + 3) as QCGs covariant with respect toSL(3,R), SL(3,R)× SL(3,R),SL(6,R),E6(6) andSO(n,m)× SO(1, 1), respectively, their spherical vectors andquadratic Casimir operators.

I For ν = −(nV + 2) + iρ the quasiconformal action inducesunitary representations that belong to the principle series. Forspecial discrete values of ν the quasiconformal action leads tounitary representations belonging to the discrete series andtheir continuations. For the quaternionic real forms theybelong to the quaternionic discrete series.

M. Gunaydin, Istanbul,Aug. 4 2011 44

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I Unified realization of 3D U-duality groups of all N = 2MESGTs defined by Jordan algebras as spectrum generatingquasiconformal groups covariant with respect to their 5DU-duality groups. MG, Pavlyk (2009)

I The spherical vectors of quasiconformal realizations ofF4(4),E6(2),E7(−5),E8(−24) and SO(d + 2, 4) twisted by aunitary character ν with respect to their maximal compactsubgroups as well as their quadratic Casimir operators

I Unified realization of F4(4),E6(6),E7(7),E8(8) and ofSO(n + 3,m + 3) as QCGs covariant with respect toSL(3,R), SL(3,R)× SL(3,R),SL(6,R),E6(6) andSO(n,m)× SO(1, 1), respectively, their spherical vectors andquadratic Casimir operators.

I For ν = −(nV + 2) + iρ the quasiconformal action inducesunitary representations that belong to the principle series. Forspecial discrete values of ν the quasiconformal action leads tounitary representations belonging to the discrete series andtheir continuations. For the quaternionic real forms theybelong to the quaternionic discrete series.

M. Gunaydin, Istanbul,Aug. 4 2011 44

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Minimal Unitary Representations and QuasiconformalGroups

I Quantization of the quasiconformal realization of anon-compact Lie group leads directly to its minimal unitaryrepresentation ⇒ Unitary representation over the Hilbertspace of square integrable functions of smallest number ofvariables possible.

I Minimal unitary representation of E8(−24) over L2(R29) fromits geometric realization as a quasiconformal group MG, Pavlyk, 2004

E8(−24) = 1−2 ⊕ 56−1 ⊕ E7(−25) + SO(1, 1)⊕ 56+1 ⊕ 1+2

56 of E7(−25) ⇒ 28 coordinates and 28 momenta. These 28coordinates plus the singlet coordinate yield the minimalnumber of variables for E8.

M. Gunaydin, Istanbul,Aug. 4 2011 45

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QCG Approach to Minimal Unitary RepresentationsLie algebra g of a QCG G can be realized as follows:

I

g = g−2 ⊕ g−1 ⊕ (h⊕∆)⊕ g+1 ⊕ g+2

g = E ⊕ Eα ⊕ (Ja + ∆)⊕ Fα ⊕ F

∆ determines the 5-grading and α, β, .. = 1, 2, ..., 2n

E =1

2y 2 Eα = y ξα, Ja = −1

2λaαβξ

αξβ

F =1

2p2 +

κI4(ξα)

y 2, Fα = [Eα,F ][

ξα , ξβ]

= Ωαβ = −Ωβα, [y , p] = i

I4(ξα) = Sαβγδξαξβξγξδ ⇔ quartic invariant of h = g0/∆

Minimal Gelfand-Kirillov dimension for a unitaryrepresentation =n + 1

M. Gunaydin, Istanbul,Aug. 4 2011 46

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4D, N = 2 σ-models coupled to Supergravity in HarmonicSuperspace and Minimal Unitary Representations

Galperin, Ogievetsky 1993

I In HSS the metric on a quaternionic target space is given by aquartic potential L(+4). The action is

S =

∫dζ(−4)duQ+

α D++Q+α−q+i D++q+i+L(+4)(Q+, q+, u−)

ζ, u±i are analytic superspace coordinatesQ+α (ζ, u), α = 1, ..., 2n are hypermultiplets and

q+i (ζ, u), (i = 1, 2) are supergravity compensators.

Q+α and q+

i are analytic N = 2 superfields.

I ” Hamiltonian mechanics” with D++ playing the role of timederivatives and Q+ and q+ corresponding to phase spacecoordinates under Poisson brackets

f , g =1

2Ωαβ ∂f

∂Q+α

∂g

∂Q+β− 1

2εij

∂f

∂q+i

∂g

∂q+j,

M. Gunaydin, Istanbul,Aug. 4 2011 47

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4D, N = 2 σ-models coupled to Supergravity in HarmonicSuperspace and Minimal Unitary Representations

Galperin, Ogievetsky 1993

I In HSS the metric on a quaternionic target space is given by aquartic potential L(+4). The action is

S =

∫dζ(−4)duQ+

α D++Q+α−q+i D++q+i+L(+4)(Q+, q+, u−)

ζ, u±i are analytic superspace coordinatesQ+α (ζ, u), α = 1, ..., 2n are hypermultiplets and

q+i (ζ, u), (i = 1, 2) are supergravity compensators.

Q+α and q+

i are analytic N = 2 superfields.I ” Hamiltonian mechanics” with D++ playing the role of time

derivatives and Q+ and q+ corresponding to phase spacecoordinates under Poisson brackets

f , g =1

2Ωαβ ∂f

∂Q+α

∂g

∂Q+β− 1

2εij

∂f

∂q+i

∂g

∂q+j,

M. Gunaydin, Istanbul,Aug. 4 2011 47

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I Isometries are generated by Killing potentials KA(Q+, q+, u−)that obey the ”conservation law”

∂++KA + KA,L(+4) = 0

L(+4) =P(+4)(Q+)

(q+u−)2

P(+4)(Q+) = 112 Sαβγδ Q+αQ+βQ+γQ+δ

where Sαβγδ is a completely symmetric invariant tensor of H.The Killing potentials that generate the isometry group G aregiven by

Sp(2) : K ++ij = 2(q+

i q+j − u−i u−j L

(+4)),

H : K ++a = taαβQ+αQ+β,

G/H× Sp(2) : K ++iα = 2q+

i Q+α − u−i (q+u−)∂−αL(+4)

M. Gunaydin, Istanbul,Aug. 4 2011 48

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N = 2 σ-model in HSS Minrep of Isometry Grp Gw y

p++ p , i [ , ]Q+α ξα

P(+4)(Q+) I4(ξ)K a++ = taαβQ+αQ+β Ja = λaαβξ

αξβ

T +++α = T +

α ,M++++ Fα = [Eα,F ]

T +α = −

√2wQ+

α Eα = y ξα

M++++ = 12 (p++)2 − P(+4)(Q+)

w2 F = 12 p2 + κ(I4(ξα))

y2

M0 = 12 w 2 E = 1

2 y 2

M++ = 12 (wp++ + p++w) ∆ = − i

2 (yp + py)

Table: The correspondence between the harmonic superspaceformulation of N = 2 sigma models coupled to supergravity and theminimal unitary realizations of their isometry groups G obtained byquantization of quasiconformal action of G .

M. Gunaydin, Istanbul,Aug. 4 2011 49

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I The above mapping implies that the fundamental spectra ofthe ”quantum” N = 2 , quaternionic Kahler σ models coupledto sugra in d = 4 must fit into the minimal unitaryrepresentations of their isometry groups.

I The N = 2 , d = 4 MESGT’s , under dimensional reduction,lead to d = 3 supersymmetric σ models with quaternionicKahler manifolds M3 (C-map). After T-dualizing the threedimensional theory one can lift it back to four dimensions,thereby obtaining an N = 2 sigma model coupled tosupergravity that is in the mirror image of the original N = 2MESGT.

I The above results suggest that there must be acorrespondence between the fundamental and full quantumspectrum of a 4D, N = 2 MESGT and the minimal unitaryrepresentation of its three dimensional U-duality group andthose representations obtained by tensoring of its minrep.

I Important open problem: decomposition of tensor products ofminreps into irreducible representations of the spectrumgenerating symmetry groups.

M. Gunaydin, Istanbul,Aug. 4 2011 50

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I The above mapping implies that the fundamental spectra ofthe ”quantum” N = 2 , quaternionic Kahler σ models coupledto sugra in d = 4 must fit into the minimal unitaryrepresentations of their isometry groups.

I The N = 2 , d = 4 MESGT’s , under dimensional reduction,lead to d = 3 supersymmetric σ models with quaternionicKahler manifolds M3 (C-map). After T-dualizing the threedimensional theory one can lift it back to four dimensions,thereby obtaining an N = 2 sigma model coupled tosupergravity that is in the mirror image of the original N = 2MESGT.

I The above results suggest that there must be acorrespondence between the fundamental and full quantumspectrum of a 4D, N = 2 MESGT and the minimal unitaryrepresentation of its three dimensional U-duality group andthose representations obtained by tensoring of its minrep.

I Important open problem: decomposition of tensor products ofminreps into irreducible representations of the spectrumgenerating symmetry groups.

M. Gunaydin, Istanbul,Aug. 4 2011 50

Page 73: Murat Guna ydin Aug. 4, 2011 Koc University, Istanbulhome.ku.edu.tr/~sbsg/Talks/Istanbul_2011_Koc_Gunaydin.pdf · Exceptional N = 2 versus Maximal N = 8 Supergravity: I The exceptional

I The above mapping implies that the fundamental spectra ofthe ”quantum” N = 2 , quaternionic Kahler σ models coupledto sugra in d = 4 must fit into the minimal unitaryrepresentations of their isometry groups.

I The N = 2 , d = 4 MESGT’s , under dimensional reduction,lead to d = 3 supersymmetric σ models with quaternionicKahler manifolds M3 (C-map). After T-dualizing the threedimensional theory one can lift it back to four dimensions,thereby obtaining an N = 2 sigma model coupled tosupergravity that is in the mirror image of the original N = 2MESGT.

I The above results suggest that there must be acorrespondence between the fundamental and full quantumspectrum of a 4D, N = 2 MESGT and the minimal unitaryrepresentation of its three dimensional U-duality group andthose representations obtained by tensoring of its minrep.

I Important open problem: decomposition of tensor products ofminreps into irreducible representations of the spectrumgenerating symmetry groups.

M. Gunaydin, Istanbul,Aug. 4 2011 50

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AdS/CFT Aspen Summer 1984

I The Kaluza-Klein spectrum of IIB supergravity on AdS5 × S5

was first obtained via the oscillator method by simpletensoring of the CPT self-conjugate doubleton supermultipletof N = 8 AdS5 superalgebra PSU(2, 2 | 4).

I The CPT self-conjugate doubleton supermultiplet ofPSU(2, 2 | 4) of AdS5 × S5 solution of IIB supergravity doesnot have a Poincare limit in five dimensions and decouplesfrom the Kaluza-Klein spectrum as gauge modes and the fieldtheory of CPT self-conjugate doubleton supermultiplet ofPSU(2, 2 | 4) lives on the boundary of AdS5, which can beidentified with 4D Minkowski space on which SO(4, 2) acts asa conformal group, and the unique candidate for this theory isthe four dimensional N = 4 super Yang-Mills theory that wasknown to be conformally invariant. MG , Marcus (1984)

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AdS/CFT Aspen Summer 1984

I The Kaluza-Klein spectrum of IIB supergravity on AdS5 × S5

was first obtained via the oscillator method by simpletensoring of the CPT self-conjugate doubleton supermultipletof N = 8 AdS5 superalgebra PSU(2, 2 | 4).

I The CPT self-conjugate doubleton supermultiplet ofPSU(2, 2 | 4) of AdS5 × S5 solution of IIB supergravity doesnot have a Poincare limit in five dimensions and decouplesfrom the Kaluza-Klein spectrum as gauge modes and the fieldtheory of CPT self-conjugate doubleton supermultiplet ofPSU(2, 2 | 4) lives on the boundary of AdS5, which can beidentified with 4D Minkowski space on which SO(4, 2) acts asa conformal group, and the unique candidate for this theory isthe four dimensional N = 4 super Yang-Mills theory that wasknown to be conformally invariant. MG , Marcus (1984)

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I The spectra of 11D supergravity over AdS4 × S7 andAdS7 × S4 were fitted into supermultiplets of the symmetrysuperalgebras OSp(8 | 4,R) and OSp(8∗|4) constructed byoscillator methods. The entire Kaluza-Klein spectra over thesetwo spaces were obtained by tensoring the singleton anddoubleton supermultiplets of OSp(8 | 4,R) and OSp(8∗|4),respectively.

I The relevant singleton supermultiplet of OSp(8 | 4,R) anddoubleton supermultiplet of OSp(8∗|4) do not have a Poincarelimit in four and seven dimensions, respectively, and decouplefrom the respective spectra as gauge modes. Again it wasproposed that field theories of the singleton and scalardoubleton supermutiplets live on the boundaries of AdS4 andAdS7 as superconformally invariant theories. MG, Warner(1984), MG, PvN, Warner ( 1984).

I Singletons of Sp(4,R) are the remarkable representations ofDirac (1963). Subsequent important work of Fronsdal andcollaborators on the singular nature of their Poincare limit andthe massless representations of SO(3, 2) obtained by tensoringtwo singletons.

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I The spectra of 11D supergravity over AdS4 × S7 andAdS7 × S4 were fitted into supermultiplets of the symmetrysuperalgebras OSp(8 | 4,R) and OSp(8∗|4) constructed byoscillator methods. The entire Kaluza-Klein spectra over thesetwo spaces were obtained by tensoring the singleton anddoubleton supermultiplets of OSp(8 | 4,R) and OSp(8∗|4),respectively.

I The relevant singleton supermultiplet of OSp(8 | 4,R) anddoubleton supermultiplet of OSp(8∗|4) do not have a Poincarelimit in four and seven dimensions, respectively, and decouplefrom the respective spectra as gauge modes. Again it wasproposed that field theories of the singleton and scalardoubleton supermutiplets live on the boundaries of AdS4 andAdS7 as superconformally invariant theories. MG, Warner(1984), MG, PvN, Warner ( 1984).

I Singletons of Sp(4,R) are the remarkable representations ofDirac (1963). Subsequent important work of Fronsdal andcollaborators on the singular nature of their Poincare limit andthe massless representations of SO(3, 2) obtained by tensoringtwo singletons.M. Gunaydin, Istanbul,Aug. 4 2011 52

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Minimal Unitary Representations versus Singletons &Doubletons and Supersymmetry

MG, Pavlyk (2006), MG, Fernando (2009/10)

I The minimal unitary representations of symplectic groupsSp(2n,R) are the singletons and their generators can bewritten as bilinears of bosonic oscillators since their quarticinvariants vanish. Tensoring procedure becomes simple for thesymplectic groups. Minreps of OSp(2n|2m,R) aresupersingletons

I Minimal unitary representation of SU(2, 2) = SO(4, 2) over L2

functions in 3 variables ⇔ conformal scalar = scalar doubletonI Minrep of SU(2, 2) admits a one-parameter, ζ , family of

deformations corresponding to massless conformal fields ind = 4 with helicity ζ/2.

I Minrep of PSU(2, 2|4) is the 4D Yang-Mills supermultiplet(CPT-self-conjugate doubleton)

I Minrep of SU(2, 2|N) admits a one-parameter family ofdeformations ⇔ Higher spin doubleton supermultiplletsstudied in MG, Minic , Zagermann (1998).M. Gunaydin, Istanbul,Aug. 4 2011 53

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I Minrep of SO∗(8) ' SO(6, 2) realized over the Hilbert spaceof functions of five variables and its deformations labeled bythe spin t of an SU(2) subgroup correspond to masslessconformal fields in six dimensions. Minimal unitarysupermultiplet of OSp(8∗|2N) admits deformations labeleduniquely by the spin t of an SU(2) subgroup of the littlegroup SO(4) of lightlike vectors in 6D.

I Minrep of OSp(8∗|4) is the massless supermultiplet of (2, 0)conformal field theory that is dual to M-theory on AdS7 × S4.

I The above results suggest the remarkable fact that the minrepof any noncompact group G must admit deformations if itoccurs as a factor in the even subgroup G × K of asupergroup. ( For K compact such supergroups admit unitaryrepresentations.) Groups F4,E6,E7 and E8 do not occur assuch subgroups!

M. Gunaydin, Istanbul,Aug. 4 2011 54

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I Minrep of SO∗(8) ' SO(6, 2) realized over the Hilbert spaceof functions of five variables and its deformations labeled bythe spin t of an SU(2) subgroup correspond to masslessconformal fields in six dimensions. Minimal unitarysupermultiplet of OSp(8∗|2N) admits deformations labeleduniquely by the spin t of an SU(2) subgroup of the littlegroup SO(4) of lightlike vectors in 6D.

I Minrep of OSp(8∗|4) is the massless supermultiplet of (2, 0)conformal field theory that is dual to M-theory on AdS7 × S4.

I The above results suggest the remarkable fact that the minrepof any noncompact group G must admit deformations if itoccurs as a factor in the even subgroup G × K of asupergroup. ( For K compact such supergroups admit unitaryrepresentations.) Groups F4,E6,E7 and E8 do not occur assuch subgroups!

M. Gunaydin, Istanbul,Aug. 4 2011 54

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OPEN PROBLEMS

I Decomposition of tensor products of minreps of U-dualitygroups into irreps. Of particular interest are E8(8) and E8(−24).

I Physical meaning of the states of minrep of U-duality groups.For AdS supergroups the minreps act like ”quarks” of positiveenergy unitary representations → AdS/CFT

I For 3D U-duality groups of MESGTs with 8 realsupersymmetries the fundamental spectrum corresponds to”super BPS” states, i.e they preserve full susy!

I Construction of the full spectrum by tensoring of minreps andembedding into their quantum completion ( M/Superstringtheory).

I At the non-perturbative level one expects only the discretesubgroups of U-duality groups to be symmetries ofM/superstring theory compactified to various dimensions ontori or their orbifolds . How to extend the above results to thediscrete subgroups? Automorphic representations ?

M. Gunaydin, Istanbul,Aug. 4 2011 55