A D-brane is a localized RR-charged source whose long-distance fields solve supergravity. The extremal charged -brane solutions carry the same RR charges, brane tension and preserved supersymmetry as the open-string construction. For the standard asymptotically flat cases , the D-brane supergravity solution in the string frame isThe function is a positive harmonic function away from the source, in transverse dimensions. In an electric gauge, , with its orientation chosen to match the source. Magnetic branes use the dual flux; for the D3-brane, the five-form includes both electric and magnetic pieces and is self-dual. Killing spinors obey one brane projector, leaving sixteen supersymmetries. Aligned multicenter harmonic functions describe several branes with no static binding force.
To check this identification directly, insert an equally oriented static probe into the solution. Put , so the asymptotic tension is . The induced-volume factor is ; combined with , its DBI action density is . Its Wess-Zumino brane coupling contributes . Hence the total static Lagrangian density is the constant , independently of position. This gives the parallel D-brane no-force identity in the spacetime description.
The supergravity background is the back-reacted, coarse long-distance description, while the boundary-condition description exposes the light open-string degrees of freedom. Controlled use of supergravity requires curvature small in string units and suitable local coupling. Singular cores and the special codimension-two or domain-wall cases are not automatically resolved by the elementary harmonic ansatz.
Articles by others on the same topic
There are currently no matching articles.