Exact solutions in supergravity theory
James T. Liu 26 July 2005
Lecture 1: Introduction and overview of supergravity Lecture 2: Conditions for unbroken supersymmetry Lecture 3: BPS black holes and branes
Lecture 4: The LLM bubbling AdS construction
Lecture 3 Outline
• D = 11 supergravity with F(4) 6= 0
The AdS4 × S7 (Freund-Rubin) background The supergravity M2-brane
• Generalized holonomy when F(4) 6= 0
Definition of generalized holonomy A look at the M2-brane
Turning on fluxes
• We now consider the general case with charges or fluxes turned on
For example, we can consider D = 11 supergravity
∇ˆM = 0 ∇ˆM = ∇M + 2881 (ΓMN P QR − 8δMNΓP QR)FN P QR
• Different approaches to solving this system
− Ansatz based on symmetry
− Generalized holonomy
− G-structure analysis
− Combination of methods, etc.
Use of symmetry: the Freund-Rubin ansatz
• The presence of F(4) hints at a natural compactification to four dimensions, M11 = M4 × X7
dˆs211 = ds24 + ds27(X7) F(4) = m(4)
• Solve the equations of motion
F(4) eom: dF(4) = 0 and d ∗F(4) + 12F(4) ∧ F(4) = 0
⇒ m = constant
Einstein: RM N = 121 (FM N2 − 121 gM NF2) Decompose D = 11 indices:
µ, ν, . . . = 0, 1, 2, 3 m, n, . . . = 4 . . . 10
Freund-Rubin: the bosonic solution
• Use Fµν2 = −6m2gµν and F2 = −24m2 to obtain
Rµν = −3(m/3)2gµν AdS4
Rmn = 6(m/6)2gmn Einstein (e.g. S7)
• Maximum symmetry for the 4 + 7 split is
M11 = AdS4 × S7
• There are three other interesting cases
− A 7 + 4 split gives AdS7 × S4
− IIB theory with self-dual F(5) gives AdS5 × S5
− The D1-D5 system gives AdS3 × S3 × T4
Freund-Rubin: Killing spinors
• To explore supersymmetry, we reduce
∇ˆM = ∇M + 2881 (ΓMN P QR − 8δMNΓP QR)FN P QR
along the µ and m directions to obtain
∇ˆµ = ∇µ − 361 mµνρσΓνρσ
∇ˆm = ∇m + 2881 mµνρσΓmΓµνρσ Introduce Γ5 = iΓ0123
∇ˆµ = ∇µ + 2i(m/3)ΓµΓ5 ∇ˆm = ∇m − 2i(m/6)ΓmΓ5
Killing spinor in AdS Killing spinor on spheres
Freund-Rubin: Killing spinors
• The basic solution, AdS4 × S7, has maximal supersymmetry
• Of course, we could replace S7 by a manifold with reduced supersymmetry
7-dimensional Einstein manifold with ‘weak’ G2 holonomy yields N = 1 inD = 4
• Conversely, we can ask how many backgrounds there are preserving maximal supersymmetry
Answered by J. Figueroa-O’Farrill and G. Papadopoulos, JHEP 0303, 048 (2003) 1. M1,10 Flat Minkowski space
2. AdS4 × S7 Freund-Rubin 3. AdS7 × S4
4. Hpp pp-wave geometry F(4) = µ dx− ∧ dx1 ∧ dx2 ∧ dx3 ds211 = 2dx+dx− − µ2(~x2 + 14~y 2)(dx−)2 + d~x32 + d~y62
Maximal supersymmetry in D = 11
• Classification performed through integrability
Define MM N ≡ [ ˆ∇M, ˆ∇N] ≡ 14R
For maximal supersymmetry, R vanishes for all
This implies the matrix R = cMΓM + cM NΓM N + · · · + cM N P QRΓM N P QR must vanish
→ cM, cM N, . . . , cM N P QR all vanish
• Working out the consequences of these conditions is sufficient to prove the result
Use of symmetry: the M2-brane
• The 3-form potential A(3) of D = 11 supergravity couples naturally to the worldsheet of the eleven-dimensional supermembrane (M2-brane)
• The M2-brane carries mass (GM N) and charge (electric F(4))
BPS → mass = charge
• We obtain the M2 geometry by considering a longitudinal + transverse split, M11 = M3 × M8
Take the ansatz: ds211 = e2A(y)dx2µ + e2B(y)dyi2
F(4) = dx0 ∧ dx1 ∧ dx2 ∧ de2C(y)
Goal: obtain a supersymmetric solution for A(y), B(y) and C(y)
The M2-brane: supersymmetry
• We may work out the Killing spinor equations
In the longitudinal direction
∇ˆµ = ∂µ + 12ωµνiΓνi − 121 FµνρiΓνρi
= ∂µ + 16ΓµΓie−3A∂i(e3A + e2CΓ012) In the transverse direction
∇ˆi = ∂i + 14ωijkΓjk + 721 FµνρjΓiµνρj − 361 FiµνρΓµνρ
= ∂i + 16e−3A∂ie2CΓ012 + 12Γij(∂jB − 16e−3A∂je2CΓ012)
• We may build a projection by taking e3A = e2C and B = −13C
⇒ e3A = e−6B = e2C
The M2-brane: supersymmetry
• The resulting expressions for the supercovariant derivative are
∇ˆµ = ∂µ + 23ΓµΓi∂iC P+
∇ˆi = ∂i − 13∂iC − 13(Γij − 2δij)∂jC P+ where P± = 12(1 ± Γ012)
• Killing spinors are easily obtained
= e13CP−0
Note that partial supersymmetry does not imply the equations of motion . . . only that the metric and form-field are given in terms of a single function C(y)
The M2-brane: supergravity solution
• To obtain a solution, we impose (one) equation of motion
d ∗F(4) + 12F(4) ∧ F(4) = 0 → d ∗F(4) = 0 → d ∗8 de−2C = 0
Hence e−2C is harmonic in transverse space
e−2C = H = 1 + X
i
qi
|~y − ~yi|6
• The complete solution
ds211 = H−2/3dx2µ + H1/3dyi2 F(4) = dx0 ∧ dx1 ∧ dx2 ∧ d„ 1
H
«
= H−1/6P−0 Harmonic superposition for BPS objects
The M2-brane: BPS and time independence
• We may construct a vector from spinor bilinears
V µ = Γµ = H−1/30Γµ0 = 0Γµ0
A constant vector pointing in the time direction, V = ∂
∂t
ΓM = real ΓTµ = −C−1ΓµC C = Γ0 ψ = ψTC−1
• We can prove that V µ is a Killing vector
∇M = −2881 (ΓMN P QR − 8δMN ΓP QR) FN P QR
∇M = 2881 (ΓMN P QR + 8δMN ΓP QR)FN P QR
→ ∇MVN = 16FM N P QΓP Q + 6!1 ∗ FM N P QRSTΓP QRST
The supergravity p-brane ansatz
• Generalize the M2-brane solution to other objects and other dimensions
• Effective description in terms of the metric (mass M), a dilatonic scalar and an electrically charged (p + 2)-form field strength (charge Q)
e−1L = R − 12dφ ∧ ∗dφ − 12eαφF(p+2) ∧ ∗F(p+2)
F(p+2) → A(p+1) → (p + 1)-dimensional world volume → p-brane
• Ansatz
ds211 = e2A(y)dx2µ + e2B(y)dy2i
φ = φ(x) F(p+2) = dx0 ∧ . . . ∧ dxp ∧ de2C(y)
The p-brane solution
• The solution depends on the parameter ∆
a2 = ∆ − 2d ˜d D − 2
d = p + 1 (worldvolume dim) d = D − d − 2 (dual brane dim)˜
and is given by
ds2 = H−4 ˜d/∆(D−2)dx2µ + H4d/∆(D−2)dyi2
eφ = H2a/∆ F(p+2) = 2∆−1/2dx0 ∧ . . . ∧ dxp ∧ d(1/H)
• The function H is harmonic in the transverse space
H(y) = 1 + X
i
qi
|~y − ~yi|d˜
Generalized holonomy classification
• The presence of F(4) modifies the covariant derivative
∇ˆM = ∇M + 2881 (ΓMN P QR − 8δMNΓP QR)FN P QR = ∂M + 14ΩM
where
ΩM = ωMABΓAB + 721 (ΓMN P QR − 8δMNΓP QR)FN P QR is a generalized connection taking values in SL(32; R)
• Introduce Generalized holonomy H ⊆ SL(32; R) for the generalized connection ΩM
[DM(Ω), DN(Ω)] = 14RM N(Ω)
The number of preserved supersymmetries = the number of singlets in the decomposition of the 32 of SL(32; R) under H
The number of singlets
• For a 32-component spinor, we may choose a basis of Killing spinors
= 2 6 6 4
1 0 0...
3 7 7 5
2 6 6 4
0 1 0...
3 7 7 5
etc.
To preserve n supersymmetries, the generalized holonomy must act as
R ∈ 0
@ SL(32; R)
1
A →
0
@
1 Rn,32−n
0 SL(32 − n; R) 1 A
Hence H ⊆ SL(32 − n; R) n ⊕nR32−n
However H does not have to be so large, so long as the singlet counting is correct
Generalized holonomy for the Freund-Rubin background
• For the Fruend-Rubin ansatz, ∇ˆM split into
∇ˆµ = ∇µ + 2i(m/3)ΓµΓ5 ∇ˆm = ∇m − 2i(m/6)ΓmΓ5
Killing spinor in AdS Killing spinor on spheres
• Focus on the 7-sphere part Integrability yields
[ ˆ∇m, ˆ∇n] = [∇m, ∇n] − 14(m/6)2[ΓmΓ5, ΓnΓ5]
= 14[Rmnpq − (m/6)2(gmpgnq − gmqgnp)]Γpq
• Substituting in the equation of motion Rmn = 5(m/6)2gmn gives
[ ˆ∇m, ˆ∇n] = 14CmnpqΓpq
Higher order integrability
• First order integrability: [ ˆ∇m, ˆ∇n] = 14CmnpqΓpq For the round S7, the Weyl tensor vanishes
⇒ trivial generalized holonomy
Puzzle for the squashed S7:
left-squashing gives N = 1 while right-squashing gives N = 0 but first order integrability cannot distinguish these cases
• Second order integrability:
[ ˆ∇l, [ ˆ∇m, ˆ∇n]] = 14(∇lCmnabΓab − 2i(m/6)Cmnla
ΓaΓ5)
left- and right-squashing give opposite signs for m
Generalized holonomy for the squashed S
7• The generalized structure group is SO(8)
SO(7) is generated by 12iΓab;
SO(8) is generated by appending ΓaΓ5 to the above set
• At first order, we only see SO(7)
SO(7) ⊃ G2 : 8 → 7 + 1
• At second order, we see SO(8)
SO(8) ⊃ Spin(7) : 8s → 7 + 1 N = 1 for left-squashing SO(8) ⊃ Spin(7) : 8s → 8 + 1 N = 0 for left-squashing
Generalized holonomy for the M2-brane
• Given ∇ˆ M = ∂M + 14ΩM, the M2 background yields the generalized connection
Ωµ = 83∂iC(ΓµΓiP+) Ωi = 43∂iCΓ012 − 43∂jC(ΓijP+)
• We may view these as Lie algebra generators
Tij = ΓijP+ Kµ i = ΓµiP+ Kµ ijk = ΓµijkP+
where Kµ ijk arises from second order integrability
• The result is
HolM2 = SO(8)+ n 12R2(8s) ⊂ SL(16; R) n 16R16
Generalized holonomies of other objects
• A similar analysis may be performed for the basic objects of M-theory
n Background Generalized holonomy
32 E1,10, AdS7 × S4, AdS4 × S7, Hpp {1}
18,. . . ,26 plane waves R9
16 M5 SO(5) n 6R4(4)
16 M2 SO(8) n 12R2(8s)
16 MW R9
16 MK SU (2)
The M-wave and KK monopole are pure geometry solutions
• Is there a generalized holonomy classification generalizing Berger’s classification of Riemannian holonomy?
Next time
• Direct use of the Killing spinor equations in constructing new supersymmetric vacua
G-structure (Killing tensor) analysis
• The LLM construction of all 1/2 BPS bubbling AdS5 × S5 backgrounds with SO(4) × SO(4) isometry