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Gravity and Strings

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19.6 Intersections 567<br />

outside the string in the presence of other fields, the equation of motion has additional terms<br />

<strong>and</strong> the homotopy-invariant definition of charge is<br />

<br />

−2 ˆϕ⋆<br />

e ˆH − ⋆ ˆG (3) Ĉ (0) − ˆG (5) Ĉ (2) , (19.140)<br />

qF1 ∼<br />

S 7<br />

where S7 surrounds the string. Let us consider a semi-infinite string. At a large enough<br />

distance L from the endpoint, boundary effects are not important <strong>and</strong> the charge is still<br />

approximately given by the first of Eqs. (19.102). The larger L is for a fixed value of the S7 radius R7, the better the approximation. Closer to the endpoint, the additional terms must<br />

contribute (otherwise, we are back in the previous case), but we can obtain the same value<br />

for the integral by making R7 → 0keeping R7/L constant until the only contribution to the<br />

integral comes from the endpoint. The degenerate S7 can be decomposed, for convenience,<br />

into the product S5 × S2 ,ifweassume that the contribution to qF1B comes from the last<br />

term in the above integral. The integral decomposes into a product of integrals,<br />

<br />

ˆG (5)<br />

<br />

Ĉ (2) . (19.141)<br />

S 5<br />

The first integral gives the D3-brane charge (assuming, as we are doing here, that ˆH does<br />

not contribute), ˆG (5) = ⋆ ˆG (5) ,<strong>and</strong> thus the string endpoint must be at a D3-brane. If there is<br />

no D1-brane present, then, ˆG (3) ∼ dĈ (2) = 0 inside the D3-brane <strong>and</strong>, locally, Ĉ (2) = dV,<br />

where V is a vector that lives in the D3-brane worldvolume. Then<br />

<br />

qF1B ∼ dV. (19.142)<br />

The interpretation is clear: an F1B can end on a D3-brane <strong>and</strong> at the intersection point<br />

there is an excited worldvolume vector field (the dual BI vector field) whose magnetic<br />

charge is proportional to the F1B charge. This is the same result as we obtained before.<br />

Asimilar reasoning indicates that, if it is the second term that contributes to the charge<br />

integral, the F1B can also end on a D-string <strong>and</strong> at the intersection the BI vector field is<br />

excited so its dual field strength is a constant. 27<br />

These arguments that determine the opening of branes seem to depend on field redefinitions<br />

(the charge integr<strong>and</strong> is defined up to total derivatives). However, the different<br />

expressions for the charge are just choices that are more or less adequate to describe a<br />

given physical situation. The most symmetric expression for qF1B can be obtained by using<br />

Eq. (17.9). Each of the four possible terms corresponds to the F1B ending on one of the<br />

four Dp-branes p = 1, 3, 5, <strong>and</strong> 7 <strong>and</strong> exciting the dual BI field magnetically.<br />

19.6.2 Marginally bound supersymmetric states <strong>and</strong> intersections<br />

We are considering only supersymmetric brane intersections, in which the branes that intersect<br />

do not interact <strong>and</strong> are in supersymmetric equilibrium. These intersections can be<br />

27 This is similar to viewing the mass parameter of Romans’ N = 2A, d = 10 SUEGRA as the dual of the RR<br />

10-form field strength.<br />

S 2<br />

S 2

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