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Gravity and Strings

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15.1 Effective actions <strong>and</strong> background fields 431<br />

gauge group it must be the effective action of the heterotic <strong>and</strong> type-I strings (but already<br />

here the couplings of the 2-form are different in the two theories).<br />

The fields of these effective theories are given in Table 14.3. The NSNS fields are sometimes<br />

called the common sector since they occur in all of them, including the bosonic<br />

(oriented)-string theories. The fields in the common sector are the metric gµν, associated<br />

with the graviton, the KR 2-form Bµν, <strong>and</strong>the dilaton φ whose vacuum expectation value<br />

φ0 gives the string coupling constant g = e φ0 (see Eqs. (15.8) <strong>and</strong> (14.14)). The action for<br />

the common sector in the string frame to be defined below is given (in d dimensions with<br />

d = 10 <strong>and</strong> 26) by<br />

S =<br />

g2 16πG (d)<br />

N<br />

<br />

dd x √ |g| e−2φ <br />

R − 4(∂φ) 2 + 1<br />

<br />

2 H , (15.1)<br />

2 · 3!<br />

where, in our notation in which indices not shown are all antisymmetrized,<br />

H = 3∂ B (15.2)<br />

is the KR field strength, which is invariant under the gauge transformations necessary for<br />

the consistent quantization of a massless 2-form field,<br />

δB = 2∂, (15.3)<br />

where µ is an arbitrary vector field. The overall factor e−2φ is associated with the genus-0<br />

(tree-level) origin of these terms <strong>and</strong> the normalization is conventional. In particular, the<br />

factor g2 (g is defined in Eq. (14.57)) compensates the factor e−2φ0 that appears in the<br />

weak field expansion of the action around the vacuum gµν = ηµν,φ= φ0, soG (d)<br />

N can be<br />

interpreted as the d-dimensional Newton constant. Its value Eq. (19.26) can be determined<br />

by using duality arguments that relate it to the string coupling constant <strong>and</strong> the string length<br />

just as we determined the Newton constant in terms of the compactification radius of KK<br />

theory in Eq. (11.97), as we will see in Section 19.3.<br />

Observe that, up to normalization, the above action is also invariant under shifts of the<br />

dilaton field that change its vacuum expectation value <strong>and</strong> thus g, which is a free parameter.<br />

A potential for the dilaton could give it a mass <strong>and</strong> fix g, solving two problems simultaneously:<br />

the determination of g <strong>and</strong> the existence of a massless scalar that couples<br />

as the Jordan–Brans–Dicke field to all kinds of matter, inducing violations of the equivalence<br />

principle [287, 288]. The massless KR 2-form that also couples to matter can also<br />

be a source of violations of the equivalence principle. The KR 3-form field strength can<br />

be understood as a completely antisymmetric dynamical torsion field, as we discussed on<br />

page 132 <strong>and</strong>, in the same spirit, the dilaton can be understood as part of a non-metricity<br />

tensor of the type considered by Weyl [834]. The above string effective action can then be<br />

written as an Einstein–Hilbert action for a torsionful <strong>and</strong> non-metric-compatible connection<br />

using Eq. (1.55) (see also Eq. (1.58)).<br />

The RR fields are differential forms C (n) µ1···µn of even (odd) rank in the N = 2B (A)<br />

theory <strong>and</strong> appear in the respective actions Eqs. (17.4) <strong>and</strong> Eq. (16.38) with no couplings

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