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Gravity and Strings

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19.2 String-theory extended objects from effective-theory solutions 541<br />

either as a scalar (<strong>and</strong> then its Hodge dual, the RR 7-form Ĉ (7) ,has to be treated as a pseudotensor)<br />

or as a pseudoscalar (<strong>and</strong> the RR 7-form Ĉ (7) has to be treated as a tensor). 11 The<br />

second option (which is also the one we adopted for consistency when we defined the magnetic<br />

RR potentials) was chosen by the authors of [435], who performed the Wick rotation<br />

using the RR 7-form <strong>and</strong> treating it as a tensor. If Ĉ (0) is a pseudoscalar then it acquires an<br />

extra factor of i in the Wick rotation: Ĉ (0) = i ¯ Ĉ (0)<br />

¯S =<br />

ˆg 2 B<br />

16πG (10)<br />

N<br />

<br />

d 10 ¯ ˆx<br />

<br />

| ¯ ˆg E|<br />

¯ˆRE + 1<br />

. The Euclidean action becomes<br />

ˆϕ<br />

e2<br />

2<br />

(∂e −ˆϕ ) 2 − (∂ ¯ Ĉ (0) ) 2<br />

, (19.69)<br />

Observe that the two scalars contribute with different signs to the action. Their “energy–<br />

momentum” tensors will appear with opposite signs in the Einstein equation. Thus, one<br />

can obtain a solution with flat spacetime by taking the derivatives of the two scalars to be<br />

equal, up to a global sign. Then one need only solve the scalar equations. The D-instanton<br />

solution takes the following form in the (unmodified) Einstein <strong>and</strong> string frames [435]:<br />

d ¯ ˆs 2 E = e− ˆϕ 0 2 d ¯x 2<br />

10 , d ¯ ˆs 2 s = H 1 2<br />

Di d ¯x 2<br />

10 ,<br />

e −2 ˆϕ = e −2 ˆϕ0 H −2<br />

Di ,<br />

HDi = 1 + hDi<br />

.<br />

|¯x 8<br />

10|<br />

¯ Ĉ (0) =±e −ˆϕ0<br />

H −1<br />

Di − 1 ,<br />

(19.70)<br />

The value of hDi is the extrapolation to p =−1ofthe value of hDp Eq. (19.65). This<br />

value can also be obtained via a T-duality relation with the D0-brane.<br />

At first sight there is a singularity at ρ =|¯x 10|=0 (in the string frame). However, the<br />

string metric is invariant under the reparametrization<br />

ρ = h 1 4<br />

Di / ˜ρ, (19.71)<br />

which shows that, in the limit ρ → 0, one finds another asymptotically flat region identical<br />

to the one at ρ →∞. The metric, therefore, describes a sort of Euclidean wormhole joining<br />

the two asymptotically flat regions <strong>and</strong> is regular everywhere.<br />

The value of the Euclidean action of the D-instanton can be calculated. In the modified<br />

Einstein frame, <strong>and</strong> normalized in our conventions, it takes the value<br />

I = 2π/gB = qDi/gB. (19.72)<br />

The action Eq. (19.68) appears in other contexts in d = 10 dimensions. We have met it,<br />

for instance, as a truncation of the N = 4, d = 4SUEGRA theory that arises in the toroidal<br />

reduction of the heterotic-string effective action Eq. (16.160), but it appears in many other<br />

reductions, as shown in [666]. It is possible to find instanton solutions for all of them that<br />

are almost identical with the D-instanton solution, differing only in the harmonic function<br />

which, in d > 2 dimensions, will be H = 1 + h/|xd| d−2 . The string-frame geometry will<br />

11 This difference between these two options can be seen as the reason why Wick rotations <strong>and</strong> Hodge duality<br />

do not commute.

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