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Gravity and Strings

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T = 0<br />

1.3 Metric spaces 11<br />

Affinely Connected Metric Spacetime<br />

Riemann–Cartan Spacetime<br />

U d<br />

Riemann Spacetime Weitzenbock Spacetime<br />

V d<br />

R = 0<br />

(L ,g)<br />

d<br />

Minkowski Spacetime<br />

M d<br />

Fig. 1.1. Particular structures in an affinely connected spacetime equipped with a metric<br />

(Ld, g).<br />

There is another way of reducing the number of independent fields: by imposing<br />

the vanishing of the curvature tensor. In this case, both the metric <strong>and</strong> the connection<br />

are completely determined by the Vielbein (to be defined latter). The connection<br />

is called Weitzenböck connection [944, 945] <strong>and</strong> has torsion (also determined by the<br />

Vielbein). A Riemann–Cartan spacetime with Weitzenböck connection is a Weitzenböck<br />

spacetime Ad.<br />

If both torsion <strong>and</strong> curvature vanish, the space has to be Minkowski spacetime Md since<br />

the Minkowski metric gµν = ηµν is the only one that makes the full Riemann tensor vanish<br />

in the absence of torsion.<br />

The diagram in Figure 1.1 summarizes the different particular structures that we can have<br />

on an affinely connected manifold equipped with a metric [522, 523].<br />

In the rest of this section we are going to study the particular properties of some of these<br />

spacetimes. The Weitzenböck spacetime will be studied after the introduction of Vielbeins<br />

in Section 1.4.<br />

1.3.1 Riemann–Cartan spacetime Ud<br />

As has been said, this is an affinely connected metric spacetime with a metric-compatible<br />

connection, so the non-metricity tensor vanishes, Qµνρ = 0. According to the general result,<br />

Q = 0<br />

R = 0<br />

T = 0<br />

A d

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