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Gravity and Strings

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124 Action principles for gravity<br />

Furthermore, we are not going to assume in our derivation of the equations of motion either<br />

the symmetry of the connection or the symmetry of the “metric,” which we will impose<br />

at the very end. In this way, we can obtain with a minimum extra work the equations of<br />

the Einstein–Straus–Kaufman [358, 364, 367, 369] non-symmetric gravity theory (NGT)<br />

which was (unsuccessfully) proposed as a unified relativistic theory of gravitation <strong>and</strong> electromagnetism<br />

in which the antisymmetric part of the “metric” g [µν] should be identified<br />

with the electromagnetic field strength tensor 4 F µν .<br />

In the NGT the inverse “metric” is also denoted by g µν <strong>and</strong> satisfies<br />

g µν gνρ = δ µ ρ, gαβ g βγ = δα γ , (4.60)<br />

but g µνgµρ = δν ρ. Also, we cannot use it to lower or raise indices.<br />

Let us now vary the above action with respect to the metric <strong>and</strong> connection. By using<br />

Palatini’s identity Eq. (3.286), we find<br />

<br />

δS = dd x δgαβ Rαβ(Ɣ) + gαβ∇αδƔρβ ρ −∇ρδƔαβ ρ − Tαρ σ δƔσβ ρ<br />

<br />

=<br />

dd x δgαβ <br />

ρβ Rαβ(Ɣ) +∇ρ g δσ α − gαβδσ ρ <br />

σ<br />

δƔαβ<br />

+ ∇σ g αβ −∇ρg ρβ δσ α − g λβ Tλσ α δƔαβ σ .<br />

Using now the identity for vector densities<br />

(4.61)<br />

∇µv µ = ∂µv µ + v µ Tµρ ρ , (4.62)<br />

<strong>and</strong> integrating by parts, we obtain, up to a total derivative<br />

<br />

δS = dd x δgαβRαβ(Ɣ) + Tρδ δgρβδσ α − gαβδσ ρ<br />

+∇σ g αβ −∇ρg ρβ δσ α − g λβ Tλσ α δƔαβ σ .<br />

(4.63)<br />

Since the metric <strong>and</strong> the connection are independent, we obtain two equations from the<br />

minimal action principle:<br />

δS<br />

δgαβ = Rαβ(Ɣ) = 0,<br />

δS<br />

δƔαβ γ =∇γgαβ −∇ρgρβδγ α − gλβ Tλγ α + gρβδγ αTρδ δ − gαβ Tγδ δ (4.64)<br />

= 0.<br />

The first equation would be the Einstein equation if the connection were the Levi-Cività<br />

connection. Observe that, if we couple bosonic (scalar or vector) matter minimally to this<br />

4 See also [654, 837, 838, 895]. A more recent NGT that reinterprets Einstein’s theory was proposed in<br />

[699]. In it the antisymmetric part of the metric is also considered as a sort of new gravitational interaction.<br />

Clearly, the weak-field limit cannot be the Fierz–Pauli theory but contains another field corresponding to<br />

the antisymmetric part of the metric. While this suggests a relation with string theory, which also contains<br />

a rank-2 antisymmetric tensor (the Kalb–Ramond field), these two fields appear in quite different ways: the<br />

Kalb–Ramond field has an extra gauge symmetry, which allows it to be consistently quantized, whereas the<br />

antisymmetric part of the NGT “metric” transforms only under GCTs. See [253, 285, 286, 616].

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