Orientifolds & Twisted KR Theory

Background charge, over the integers

Jacques Distler

University of Texas at Austin

Why Orientifold?

Like orbifolds: procedure for generating new string theory backgrounds from old.

Has proven very useful for model building: IIB (and IIA) orientifold, “with fluxes” (KKLT et al …).

  • Evades the Gibbons-Maldacena-Nuñez Theorem because orientifold fixed-planes have negative tension, violating the SEC.
  • We think we understand moduli stabilization in this context.

Key feature: orientifolds have “background” D-brane charge. On a compact space, must be cancelled for consistency (Gauss’s Law).

Question

Is it possible to cancel the background charge rationally, but not cancel it over ? I.e., could the uncancelled charge be pure torsion?

Sure. But to answer the question, need to know what the background charge is over .

So far, it has only ever been computed rationally (modulo torsion). Joint work with Dan Freed and Greg Moore to rectify that.

N.b.: This is a topological question. Do not assume unbroken SUSY, or even a solution.

Subsidiary objective: clean up a bit of the bestiary of Orientifolds.

Bottom Line

  1. Background orientifold charge, μ (or μˇ), takes values in twisted (differential) KR theory.

  2. Only after inverting 2 does the formula for the background charge localize to the f.p.s.

  3. Taking Chern characters, can compare with existing formulæ in the literature

    (d+u 1 H)G=jˇD-branes+μˇorientifold
    (d+ u^{-1} H\wedge) G = \underset{\text{D-branes}}{\underbrace{\check{j}}} + \underset{\text{orientifold}}{\underbrace{\check{\mu}}}

    N.b.: putting the HG term on the RHS, as is often done is morally wrong!

Orientifold

 IIBIIA
X 10-manifoldw 1 (X)=0 Xoriented w 2 (X)=0 Xspinw 1 2 (X)+w 2 (X)=0 Xpin
σ:Xorientation-preserving, with lift to Spinlift to Pin

Let F be f.p.s. of σ (could be all of X, or could be empty).

A priori:
σ orientation-preserving codim(F)=even.
σ orientation-reversing codim(F)=odd.
In fact:
lift to Spin or to Pin codim(F) well-defined mod(4 ).

Accompany σ by reversal of orientation on worldsheet.

Generalization

Let Γ be a group of symmetries acting on X (lifting to Spin or Pin ) and let

Ω:Γ 2
\Omega: \Gamma\to \mathbb{Z}_2

be a homomorphism. Can “orientifold by Γ”, where elements of Γ which map nontrivially under Ω are accompanied by reversal of orientation on worldsheet.

N.b.: Γ can be nonabelian, even if the “orbifold subgroup,” H=kerΩΓ is abelian.

Abelian Gauge Theory

RR fields in String Theory: an exotic type of abelian gauge theory.

Recall electromagnetism.

  • j eH cpt d1 (X), j mH cpt 3 (X).
  • Electromagnetic field trivializes these: dF=j m,d*F=j e.
  • In quantum theory, need Dirac quantization condition.

𝒳 X S

RR field: replace de Rham cohomology by generalized cohomology theory, E . Dirac condition: integrality of bilinear form

b(,):E ×E H 2 (S)
b(\cdot,\cdot): E^\bullet\times E^\bullet \to H^2(S)

Self-Duality

In self-dual theory, electric current determines magnetic current (and vice versa).

j E=θ(j M)
j_E = \theta(j_M)

where θ:E E d+2 is an isomorphism.

To define the quantum theory, need a quadratic refinement, q(), of the bilinear form

b(x 1 ,x 2 )=q(x 1 +x 2 )q(x 1 )q(x 2 )(q(0 )=0 )
b(x_1,x_2) = q(x_1+x_2)- q(x_1) -q(x_2)\qquad (q(0)=0)

The Center

A quadratic function is symmetric about its center. Let ψ(x)=q(x)q(x), a linear function. Since b(,) is a perfect pairing, ψ(x)=b(λ,x) for some λ.

q(λ)=q(0 )=0
q(\lambda) = q(0) =0

The center of q is μ such that 2 μ=λ. This determines μ up to 2-torsion. Can do better, but this will suffice for today’s lecture.

Type I is an orientifold of IIB (with trivial σ action). The charge group is KR 0 (X)=KO 0 (X). Freed and Hopkins wrote down q() and computed its center

μ=T+22
-\mu = T + 22

which is, indeed, the background charge of this orientifold. (Compare with heterotic dual.)

Objective: generalize this.

Differential Cohomology

Hˇ q(X): add geometrical data to topological data in H q(X,).

Examples:

  • Hˇ 0 (X)=H 0 (X,)
  • Hˇ 1 (X)=Maps(X,S 1 ): circle-valued scalar, φ. ω=dφ closed 1-form, de Rham representative of a class in H 1 (X,).
  • Hˇ 2 (X)={isom(L,)}: c(L)H 2 (X,), the first Chern class of L. F=dA a de Rham representative of c(L).
  • etc.

Exact Sequences

More generally, the differential cohomology groups, Hˇ q(X), fit into the exact sequences

0 H q1 (X,/)flatHˇ q(X)Ω closed, q(X)0 0 Ω q1 (X)/Ω closed, q1 (X)topologically trivialHˇ q(X)H q(X,)0
\begin{gathered} 0\to \overset{\text{flat}}{\overbrace{H^{q-1}(X,\mathbb{R}/\mathbb{Z})}} \to\check{H}^q(X)\to\Omega^q_{\text{closed},\mathbb{Z}}(X)\to 0\\ 0\to\underset{\text{topologically trivial}}{\underbrace{\Omega^{q-1}(X)/\Omega^{q-1}_{\text{closed},\mathbb{Z}}(X)}} \to\check{H}^q(X)\to H^q(X,\mathbb{Z})\to 0 \end{gathered}

N.b.: Ω closed, q1 (X) is the group of gauge transformations.

Differential K-Theory

Similarly, for Kˇ q(X).

0 K q1 (X,/)Kˇ q(X)Ω closed, q(X,R)currents0 0 Ω q1 (X,R)/Ω closed, q1 (X,R)RRfieldstrengthKˇ q(X)K q(X)0
\begin{gathered} 0\to K^{q-1}(X,\mathbb{R}/\mathbb{Z})\to\check{K}^q(X)\to \overset{\text{currents}}{\overbrace{\Omega^q_{\text{closed},\mathbb{Z}}(X,R)}} \to 0\\ 0\to \underset{RR field strength}{\underbrace{\Omega^{q-1}(X,R)/\Omega^{q-1}_{\text{closed},\mathbb{Z}}(X,R)}}\to\check{K}^q(X)\to K^q(X)\to 0 \end{gathered}

where R=K (pt)=[u,u 1 ],deg(u)=2 and

0 K q(X,)/K q(X)K q(X,/)K tors q+1 (X)0
0\to K^q(X,\mathbb{R})/K^q(X)\to K^q(X,\mathbb{R}/\mathbb{Z})\to K^{q+1}_{\text{tors}}(X)\to 0

K Theory

Will help to have a specific model in mind.

Usually think of K 0 as represented by formal differences of vector bundles E 0 E 1 . Instead, consider 2 -graded vector bundles E=E 0 E 1 with an odd, skew-adjoint endomorphism, T (requires a Hermitian metric on E — a contractible choice).

Some applications will require E -dimensional and T Fredholm.

Cliff n ± (real Clifford algebra):
γ iγ j+γ jγ i=±2 δ ij,i,j=1 ,,n
K ±n:
a pair, (E,T), as before, carrying a left Cliff n ± action, which graded-commutes with T (the γ i are odd).

KR Theory

KR theory:
σ:X. Consider complex, 2 -graded vector bundles, EX, s.t. σ lifts to an even, antilinear action on fibers, which commutes with T and with the Clifford action. K-theory of such gadgets is called KR theory.

N.b., if σ acts trivially, this is just an antilinear involution for the fibers, i.e. a real structure KOtheory.

Equivariant K-theory, K G (X):
G acts on X, lifts to an even linear action on E, which commutes with T and with the Clifford action.
Hybrid, KΓ Ω:
Ω:Γ 2
lift of γΓ is even-linear or -antilinear, depending on whether Ω(γ) is nontrivial.

Twisted KR Theory

Freed-Hopkins-Teleman model for twisting K-theory (and its variants).

Isomorphism classes of twistings of KR given by the central extension

0 H 2 3 (X,˜)[Twist KR(X)]H 2 1 (X, 2 )0
0 \to H^3_{\mathbb{Z}_2}(X,\tilde{\mathbb{Z}})\to [Twist_{KR}(X)] \to H^1_{\mathbb{Z}_2}(X,\mathbb{Z}_2)\to 0

H 2 3 (X,˜) are B-fields; H 2 1 (X, 2 ) is a local version1 of (1 ) F L.

Under tensor product of twisted bundles, twistings add with the law

(η 1 ,κ 1 )+(η 2 ,κ 2 )=(η 1 +η 2 ,κ 1 +κ 2 +β˜(η 1 η 2 ))
(\eta_1,\kappa_1)+(\eta_2,\kappa_2)=(\eta_1+\eta_2,\kappa_1+\kappa_2 +\tilde{\beta}(\eta_1\cup\eta_2))

where (η i,κ i)H 2 1 (X, 2 )×H 2 3 (X,˜) and β˜ is the Bockstein β˜:H 2 2 (X, 2 )H 2 3 (X,˜) associated to 0 ˜×2 ˜ 2 0


  1. There are “universal” twistings pulled back from H 2 3 (pt,˜)H 2 1 (pt, 2 ). Depending on codim(F)mod4 , only 2 of 4 are consistent, and lead to Op ±.

Integration

𝒳 X S

Integration in equivariant KO-theory given by Dirac Index (for families).

X:KO 2 n(𝒳)KO 2 ndimX(S)
\int_X: KO_{\mathbb{Z}_2}^n(\mathcal{X})\to KO_{\mathbb{Z}_2}^{n-dim X}(S)

I’ll take a shortcut: consider 12-manifold (2-parameter family). So we map KO 2 0 KO 2 12 (pt)=KO 4 (pt)RO( 2 )=ϵ

Quadratic Refinement

Let xKR 0 +τ(X) (IIB) or xKR 1 +τ(X) (IIA). Can lift xx¯ to KO 2 0 (X). Then we integrate over a 12-manifold, and pick off the coefficient of ϵ in the result.

q(x)=( 𝒳xx¯) ϵ
q(x) = \left.\left(\int_{\mathcal{X}} x\overline{x}\right)\right|_\epsilon

The center (or, rather, twice the center) can be computed from

ψ(x)=( 𝒳((xx¯) +(πxπx¯) +)) ϵ
\psi(x) = \left.\left(\int_{\mathcal{X}}( {(x\overline{x})}_+ - {(\pi x \overline{\pi x})}_+)\right)\right|_\epsilon

Localization

After inverting 2, the formula for ψ(x) localizes to the f.p.s, F

ψ(x)= F KO[1 /2 ]2 ψ 2 (x F)Δ(ν)
\psi(x) = \int^{KO[1/2]}_F \frac{2\psi_2(x|_F)}{\Delta(\nu)}

where Δ(ν) is the spinor bundle of the normal bundle, and ψ 2 (V)=Sym 2 V 2 V is the Adams operation.

In KO[1 /2 ], ψ 2 has an inverse, ψ 1 /2 ,1 with which we can write

ψ(x)=2 F KOψ 2 (x Fψ 1 /2 (Δ(ν)))
\psi(x) = 2\int^{KO}_F \psi_2\left( \frac{x|_F}{\psi_{1/2}(\Delta(\nu))}\right)

  1. Use splitting principle and the fact that ψ 2 is a ring homomorphism. ψ 2 (L)=L 2 . Let L=1 +x, with x nilpotent. (Note: only powers of 2 in the denominators!)

    ψ 1 /2 (L)=(1 +x) 1 /2 =1 +1 2 x1 8 x 2 +1 16 x 3
    \psi_{1/2}(L) = (1+x)^{1/2} = 1 + \tfrac{1}{2} x - \tfrac{1}{8} x^2 + \tfrac{1}{16} x^3 - \dots

Cannibalistic Class

The Bott Cannibalistic Class is the KO analogue of the Wu class

M KO[1 /2 ]ψ 2 (y)= M KO[1 /2 ]yρ(M)
\int^{KO[1/2]}_M \psi_2(y) = \int^{KO[1/2]}_M y \cup \rho(M)

It can be written as (at least, for M even-dim and spin)

ρ(M)= i=1 dim(M)/2 (l i 1 /4 l i 1 /4 )=ψ 1 /2 (Δ(M))
\rho(M)= \prod_{i=1}^{dim(M)/2} \left(l_i^{1/4}\oplus l_i^{-1/4}\right) = \psi_{1/2}(\Delta(M))

where we used the splitting principle

TM= i=1 dim(M)/2 (l il i 1 )
TM\otimes\mathbb{C} = \oplus_{i=1}^{dim(M)/2} (l_i\oplus l_i^{-1})

The Background Charge (after inverting 2)

Using this, we can finally write (i:FX)

μ=i *μ F,μ F=ψ 1 /2 (Δ(F)Δ(ν))
\mu = - i_*\mu_F,\qquad \mu_F= \psi_{1/2}\left(\frac{\Delta(F)}{\Delta(\nu)}\right)

Note that, even though, in the derivation I presented, I assumed that F was spin, the ratio, Δ(F)/Δ(ν), makes sense even when neither the numerator nor the denominator makes sense separately (say, because F is only Spin ).

To compare with the existing formulæ we take Chern characters. The coupling to the RR “connection” is

XCCh(μ)Â(X) = Fi *CCh(μ F)i *Â(X)Â(ν) = Fi *CCh(μ F)Â(F)Â(ν)
\begin{aligned} \int_X C\wedge Ch(\mu) \sqrt{\hat{A}(X)} &= \int_F i^*C\wedge \frac{Ch(\mu_F)i^*\sqrt{\hat{A}(X)}}{\hat{A}(\nu)}\\ &=\int_F i^*C\wedge Ch(\mu_F) \sqrt{\frac{\hat{A}(F)}{\hat{A}(\nu)}} \end{aligned}

Scruca-Serone

It’s now a very pretty little computation1, using the splitting principle, to check that this is

2 5 codim(F) Fi *CL(R F/4 )L(R ν/4 )
-2^{5-codim(F)} \int_F i^*C \wedge\sqrt{\frac{L(R_F/4)}{L(R_\nu/4)}}

which agrees with the standard formulæ that you find in the physics literature.


  1. You’ll need the characteristic polynomials Â(R)=x i/2 sinh(x i/2 ) and L(R)=x itanh(x i).

So What?

After inverting 2, I presented you with a pretty nice, computable formula for the background charge

μ=i *(ψ 1 /2 (Δ(F)Δ(ν)))
\mu = - i_* \left(\psi_{1/2}\left(\frac{\Delta(F)}{\Delta(\nu)}\right)\right)

Though we’ve lost 2-torsion, there are still interesting examples (with 3-torsion, etc) where one can compute this explicitly.

Can be generalized to cases with non-torsion flux (H0 rationally). “RR flux” is not a separate issue. From our point of view:

  • You prescribe H (which determines what twisted KR theory we need).
  • You compute μˇ.
  • You prescribe jˇ.
  • If μ+j is trivial in the relevant twisted KR group, then you can solve for the RR field. Multiple solutions ⇔ “choices of RR flux”
  • If it’s nontrivial, then no solution for G (over !). The background is inconsistent.

Destructive String Theory

As I alluded, these consideration may, in fact, rule out some previously proposed string backgrounds.

If not, it certainly should be considered as a check on newly proposed ones.

There are a number of variations on the basic orientifold construction (Op +,Op˜ ,Op˜ +,) to which we should extend our results

The rubric of twisted (differential) KR-theory seems to be a powerful organizing principle for this bestiary of orientifolds. Perhaps you’ll find some of the ideas to be useful in other contexts as well.