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Gravity and Strings

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14<br />

String theory<br />

In this chapter we start the study of the extended objects that appear in the non-perturbative<br />

spectrum of string theory, the subject of the third part of this book. In this part we will make<br />

use of all the techniques we have developed in the first <strong>and</strong> second parts, whose main goal<br />

wastoserve as a preparation for the third.<br />

In a certain sense, this third part also presents the synthesis <strong>and</strong> (it is hoped) culmination<br />

of the ideas presented in the previous two in the framework of string theory: on the<br />

one h<strong>and</strong>, string theory includes a presumably consistent theory of quantum gravity that<br />

contains the gravitons described at lowest order by the Fierz–Pauli theory we studied in<br />

Chapter 3 [833, 834]. There are two main differences from the non-renormalizable theory<br />

of GR: the presence of a dimensionless coupling constant different from the Planck length<br />

<strong>and</strong> the presence of terms of higher order in derivatives. Furthermore, consistent string<br />

theories have spacetime supersymmetry <strong>and</strong>, therefore, supergravity, which we studied in<br />

Chapters 5 <strong>and</strong> 13. On the other h<strong>and</strong>, string theory incorporates naturally extra dimensions<br />

that have to be compactified. Thus, the ideas of Kaluza <strong>and</strong> Klein studied in Chapter 11 are<br />

also integrated into the picture.<br />

Finally, the Schwarzschild, Reissner–Nordström, pp-wave, etc. solutions studied in other<br />

chapters are also solutions of string theory <strong>and</strong> it is natural to try to use them to solve the<br />

puzzles that arise when one tries to do quantum mechanics in those backgrounds: the information<br />

<strong>and</strong> entropy problems. If string theory is really a good theory of quantum gravity,<br />

then it should help us to solve them <strong>and</strong> we will see to what extent it succeeds in the last<br />

chapter (Chapter 20) of this part.<br />

The attempts to solve these long-st<strong>and</strong>ing problems have been made possible by recent<br />

developments in string theory (essentially dualities <strong>and</strong> D-branes) <strong>and</strong> also by a change of<br />

perspective that we could call the “spacetime approach,” which is based on the effectivefield<br />

theories, when further advance with the “worldsheet approach” was becoming increasingly<br />

difficult <strong>and</strong> slow. Of course, the two approaches are complementary <strong>and</strong> there has<br />

been a considerable amount of feedback between them. In fact, some of the most interesting<br />

things that we have learned in this period are the relations between the two of them. The<br />

logic of these relations is represented schematically in Figure 14.1 <strong>and</strong> it is worth pausing<br />

for a moment to describe it in detail.<br />

405

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