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Gravity and Strings

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19<br />

The extended objects of string theory<br />

After the general introduction to extended objects of the preceding chapter, in this one<br />

we are going to study specifically the extended objects that appear in string theory. The<br />

existence of these objects is implied by our previous knowledge of existing objects (strings<br />

<strong>and</strong> Dp-branes) combined with duality. This path will be followed in Section 19.1, in which<br />

we will arrive at the diagrams in Figures 19.4.1 <strong>and</strong> 19.4.1 that represent, respectively,<br />

more- <strong>and</strong> less-conventional extended string/M-theory objects <strong>and</strong> their duality relations.<br />

The duality relations can be used to find the masses of all these objects compactified on tori<br />

(Tables 19.1–19.3) using as input the mass of a string wound once on a circle (i.e. the mass<br />

of a winding mode). To obtain consistent results (in particular for electric–magnetic dual<br />

branes to coexist satisfying the Dirac quantization condition), the ten-dimensional Newton<br />

constant has to have a specific value in terms of the string coupling constant <strong>and</strong> the string<br />

length that we will determine.<br />

The next step (Section 19.2) will be to identify which are, among the general solutions<br />

of the p-brane a-model, those that represent the long-range fields of the basic extended<br />

objects of string <strong>and</strong> M theory that we found before. We will first identify families of<br />

solutions <strong>and</strong> then we will study one by one the most important solutions. In Section 19.3<br />

we will check the values of the integration constants of those solutions against the masses<br />

<strong>and</strong> charges of the extended objects that we determined using duality arguments. Then, the<br />

duality relations between the solutions will be checked in Section 19.4.<br />

Next, in Section 19.5 we will learn how a great deal of information about all these objects<br />

is encoded in the spacetime superalgebras of the effective (supergravity) theories. In<br />

particular, the superalgebras tell us (up to a point) which extended objects may exist <strong>and</strong> the<br />

amount of unbroken supersymmetry preserved by each of them (always half of the total),<br />

as we will check by solving explicitly the Killing-spinor equations (Section 19.5.1).<br />

In Section 19.6 we will study the possible intersections between several of these objects.<br />

The worldvolume fields of the extended objects contain a large amount of information<br />

about these intersections <strong>and</strong> we will briefly review the worldvolume theories of the extended<br />

objects of string/M theory first. We will construct solutions describing the simplest<br />

intersections, which will be used in Chapter 20 to construct four-dimensional BH solutions.<br />

Some general references with emphasis on p-brane solutions of the string/M-theory effective<br />

actions are [333, 337, 417, 858, 862, 863, 901, 966]. The st<strong>and</strong>ard general refer-<br />

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