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Gravity and Strings

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3.4 The Fierz–Pauli theory in a curved background 105<br />

The first thing we have to do is to exp<strong>and</strong> this equation in powers of the perturbation hµν.<br />

The perturbation can be treated as a tensor on the background manifold. Then, it is natural<br />

to lower <strong>and</strong> raise its indices (<strong>and</strong> those of all tensors) with the background metric ¯gµν <strong>and</strong><br />

its inverse ¯g µν .Inparticular, h µν =¯g µρ ¯g νσ hρσ is not the inverse of hµν (which need not<br />

exist) <strong>and</strong> we also define h =¯g µν hµν. All barred covariant derivatives are also taken with<br />

respect to the background metric’s Levi-Cività connection ¯Ɣµν ρ .Wefind<br />

g µν =¯g µν − h µν + O(h 2 ),<br />

Ɣµν ρ = ¯Ɣµν ρ + γµν ρ + O(h 2 ),<br />

Rµνρ σ = ¯Rµνρ σ + 2 ¯∇[µγν]ρ σ + O(h 2 ),<br />

(3.281)<br />

with<br />

γµν ρ = 1<br />

2 ¯gρσ <br />

¯∇µhσν + ¯∇νhµσ − ¯∇σ hµν . (3.282)<br />

This equation is essentially the equation that gives the variation of the Levi-Cività connection<br />

δƔµν ρ (≡ γµν ρ ) under an arbitrary variation of the metric53 δgµν (≡ hµν),<br />

δƔµν ρ = 1<br />

2 gρσ <br />

∇µδgσν +∇νδgσρ −∇σδgµν . (3.284)<br />

Now we can find the expansion of Rµνρ σ to first order in hµν using the so-called Palatini<br />

identity that gives the variation of the curvature tensor under an arbitrary variation of the<br />

connection<br />

δRµνρ σ =+2∇[µδƔν]ρ σ . (3.285)<br />

The Palatini identity follows from Eqs. (1.31) <strong>and</strong> (1.36), on setting the torsion equal to<br />

zero, identifying τµν ρ with δƔµν ρ , <strong>and</strong> keeping only the linear terms. We stress that, unlike<br />

Ɣµν ρ , the variation δƔµν ρ is a true tensor <strong>and</strong> its covariant derivative is well defined. 54<br />

For the variation of Ɣµν ρ that we have just found we obtain<br />

Rµνρ σ = ¯Rµνρ σ +¯g σλ ¯∇[µ ¯∇ν]hλρ + ¯∇[µ| ¯∇ρh|ν]λ − ¯∇[µ| ¯∇λh|ν]ρ<br />

2<br />

+ O(h ), (3.287)<br />

<strong>and</strong>, on contracting the indices σ <strong>and</strong> ν,wefind55 Rµρ = ¯Rµρ + 1<br />

¯∇ 2<br />

2 hµρ − 2 ¯∇ λ ¯∇(µhρλ + ¯∇µ ¯∇ρh + O(h 2 ). (3.288)<br />

53 For further use we quote here the generalization of this equation when there is torsion present:<br />

δƔαβ γ = 1 2 gγδ <br />

∇αδgβδ +∇βδgαδ −∇δδgαβ<br />

+ 1 <br />

2 g δγ gσβδTαδ σ + g δγ gσαδTβδ σ <br />

− δTαβ<br />

γ<br />

. (3.283)<br />

54 Also for further use, here we quote the formula valid for a general connection:<br />

δRµρ =∇µδƔνρ ν −∇νδƔµρ ν − Tµν λ δƔλρ ν . (3.286)<br />

55 Sometimes the subindex L is used to indicate that the object is the part linear in hµν of the corresponding<br />

tensor with the indices in the same position. Observe that for any tensor TL µ =¯g µν TL ν <strong>and</strong> for this reason<br />

we try to avoid this notation.

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