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Gravity and Strings

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410 String theory<br />

γij. The so-called Polyakov action 5 reads<br />

SP[X µ (ξ), γij(ξ)] =− T<br />

<br />

d<br />

2 <br />

2ξ √ |γ | γ ij∂i X µ ∂ j X νgµν(X). (14.5)<br />

The general variation of this action is given by<br />

<br />

δSP = T d<br />

<br />

2ξ √ |γ | δX µ <br />

2 ν ij<br />

gµν ∇ X + γ ∂i X ρ∂ j X σ Ɣρσ ν (g) <br />

− T<br />

<br />

d<br />

2 <br />

2ξ √ |γ | δγ ij∂i X µ ∂ j X ν − 1<br />

2γijγ kl∂k X µ ∂l X νgµν <br />

− T di δX µ ∂i X νgµν. (14.6)<br />

∂<br />

Since there is no kinetic term for the worldsheet metric, its equation of motion just gives<br />

the Rosenfeld energy–momentum tensor of the worldsheet fields X µ <strong>and</strong> tells us that it<br />

must be zero. This equation is just a primary constraint that we can use to eliminate γij in<br />

the Polyakov action: on writing it in the form<br />

γkl = 2gkl/gi i , (14.7)<br />

<strong>and</strong> substituting this into the Polyakov action we recover the Nambu–Goto action. Observe<br />

that the equation of motion of the worldsheet metric γij tells us only that it is proportional<br />

to the induced metric gij,but, in just two worldsheet dimensions, it is impossible to determine<br />

the proportionality coefficient gi i = γ ijgij because this equation of motion (<strong>and</strong>,<br />

hence, the energy–momentum tensor) is (off-shell) traceless. This property is related to an<br />

additional symmetry of the Polyakov action for strings: invariance under Weyl rescalings<br />

of the worldsheet metric,<br />

γij → 2 (ξ)γij. (14.8)<br />

This symmetry plays a crucial role in the quantization of the Polyakov action, allowing<br />

one to gauge away the worldsheet metric completely <strong>and</strong> consistently: in two dimensions<br />

it is always possible to put the metric in the conformal gauge γij ∝ ηij by using<br />

reparametrizations. Then, with a Weyl rescaling, we can always obtain γij = ηij. This<br />

symmetry is, however, potentially broken by anomalies that impose further restrictions<br />

on the spacetime dimensions, metric, etc., in order to have consistent string theories (see<br />

e.g. [832]).<br />

Let us now consider the equation of motion of the X µ s. The boundary term can be nonvanishing<br />

if we consider the propagation of open strings, with free endpoints <strong>and</strong> the topology<br />

of a line segment (the alternative is to consider closed strings, with the topology of a<br />

circle). In order to eliminate it, we have to impose special boundary conditions (BCs) for<br />

open strings. There are two main possibilities (for each disconnected piece of the boundary<br />

∂ (n) <strong>and</strong> for each embedding coordinate X µ )<br />

5 It was Polyakov who first quantized it <strong>and</strong> its supersymmetric version (Eq. 14.23) using the path-integral<br />

formalism in [784, 785].

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