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String Theory and M-Theory

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396 <strong>String</strong> geometry<br />

A change in the normalization of the right-h<strong>and</strong> side would correspond to<br />

shifting the Kähler potential by an inconsequential constant. These equations<br />

show that the space spanned by wα is a Kähler manifold <strong>and</strong> the<br />

Kähler potential is given by the logarithm of the volume of the Calabi–Yau.<br />

We also define the intersection numbers<br />

<br />

καβγ = κ(eα, eβ, eγ) = eα ∧ eβ ∧ eγ<br />

(9.130)<br />

<strong>and</strong> use them to form<br />

G(w) = 1 καβγw<br />

6<br />

αwβw γ<br />

w0 = 1<br />

6w0 <br />

J ∧ J ∧ J , (9.131)<br />

which is analogous to the prepotential for the complex-structure moduli<br />

space. Here we have introduced one additional coordinate, namely w 0 , in<br />

order to make G(w) a homogeneous function of degree two. Then we find<br />

e −K1,1<br />

h<br />

= i<br />

1,1<br />

<br />

<br />

w A ∂ ¯ G ∂G<br />

− ¯wA<br />

∂ ¯w A ∂wA <br />

, (9.132)<br />

A=0<br />

where now the new coordinate w 0 is included in the sum. In Eq. (9.132) it<br />

is understood that the right-h<strong>and</strong> side is evaluated at w 0 = 1. A homework<br />

problem asks you to verify that Eq. (9.132) agrees with Eq. (9.129).<br />

The form of the prepotential<br />

To leading order the prepotential is given by Eq. (9.131). However, note that<br />

the size of the Calabi–Yau belongs to M 1,1 (M) <strong>and</strong> as a result α ′ corrections<br />

are possible. So Eq. (9.131) is only a leading-order result. However, the<br />

corrections are not completely arbitrary, because they are constrained by<br />

the symmetry. First note that the real part of w α is determined by B,<br />

which has a gauge transformation. This leads to a Peccei–Quinn symmetry<br />

given by shifts of the fields by constants ε α<br />

δw α = ε α . (9.133)<br />

Together with the fact that G(w) is homogeneous of degree two, this implies<br />

that perturbative corrections take the form<br />

G(w) = κABCw A w B w C<br />

w 0 + iY(w 0 ) 2 , (9.134)<br />

where Y is a constant. Note that the coefficient of (w 0 ) 2 is taken to be<br />

purely imaginary. Any real contribution is trivial since it does not affect the

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