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Gravity and Strings

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19.6 Intersections 571<br />

The coordinates yr = (y1 1 ,...,yr 1 ) (plus, of course, time) correspond to the common<br />

directions of the two branes relative to the worldvolume of the intersection <strong>and</strong> the solution<br />

is assumed to be independent of them. The coordinates y(p1−r) = (y2 1 ,...,y(p1−r) 2 ) <strong>and</strong><br />

y(p2−r) = (y3 1 ,...,y(p2−r) 3 ) are relative transverse coordinates (to the p1- <strong>and</strong> p2-branes,<br />

respectively). For simplicity, we will also assume the solution to be independent of them<br />

(i.e. it will be delocalized). The solution may depend only on the overall transverse coordinates<br />

(the rest), but, as we did for single-brane solutions, we include, for completeness,<br />

q additional isometries <strong>and</strong> the solution will not depend on yq. Finally, the parameters<br />

z1, z2, y1, <strong>and</strong> y2 are determined by the single-brane solutions of the a-model, Eq. (18.66).<br />

The dilaton is assumed to be a certain product of powers of H1 <strong>and</strong> H2. Finally, the Ansatz<br />

for the potentials is the usual one <strong>and</strong> we need only take into account that the pi-brane lies<br />

in the directions yr <strong>and</strong> y(pi −r):<br />

−1<br />

A(pi +1)11···r112···(pi −r)2 = αi(H i − 1), i = 1, 2. (19.149)<br />

If this Ansatz is to work, then, by insisting on the independence of the two would-be<br />

harmonic functions H1 <strong>and</strong> H2, weshould simply acquire constraints on ω,r, a1, <strong>and</strong> a2.<br />

On plugging the Ansatz into the equations of motion, we find, after a long <strong>and</strong> boring<br />

calculation, that it does indeed lead to solutions under a few conditions on those constants:<br />

ds2 = e−2a1ϕ1 H −2<br />

1<br />

1<br />

− e −2a1ϕ1 H −2<br />

1<br />

− e −2a1ϕ1 H −2<br />

1<br />

p 1 +1 e −2a2ϕ2 H −2<br />

2<br />

1<br />

1<br />

p 1 +1 e −2a2ϕ2 H −2<br />

2<br />

− 1<br />

− 1<br />

˜p 1 +1 e −2a2ϕ2 H −2<br />

2<br />

p 2 +1 Wdt 2 − d y 2<br />

r<br />

− 1<br />

− e−2a1ϕ1 H −2 ˜p 1 +1<br />

1<br />

e−2a2ϕ2 H −2<br />

2<br />

<br />

2 d y q + W −1dρ2 + ρ2d 2 <br />

(δ−2) .<br />

A(pi +1)11···r112···(pi −r)2<br />

= α1(H −1<br />

1<br />

˜p 2 +1 d y 2<br />

(p1−r)<br />

1<br />

p 2 +1 d y 2<br />

(p2−r)<br />

1<br />

− ˜p 2 +1<br />

− 1),<br />

e−2ai ϕi 2xi ≡ Hi , e−2ai ϕ −2ai ϕi −2a = e (e j ϕ j x ) j , i = j,<br />

Hi = 1 + hi<br />

ω<br />

, W = 1 + ,<br />

ρδ−3 ρδ−3 <br />

ω = hi 1 − a2 i<br />

α<br />

4xi<br />

2 <br />

<br />

i , li = (xi − 1) ci(r + 1) − p <br />

j + 1<br />

,<br />

˜pi + 1<br />

i = j,<br />

xi = (a2 i /2)ci<br />

1 + (a2 i /2)ci<br />

, ci = (pi + 1) + ( ˜pi + 1)<br />

(pi + 1)( ˜pi + 1) ,<br />

a1a2 =−2(r − r0), r0 = (p1 + 1)(p2 + 1)<br />

− 1.<br />

d − 2<br />

(19.150)<br />

This solution generalizes to the non-extreme regime extreme intersecting solutions obtained<br />

in [51] in another (a1–a2) model (see also [50, 925] <strong>and</strong> references therein). Some<br />

l i

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