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The Principle of General Covariance and the Principle of ...

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sic equation<br />

In <strong>the</strong> absence <strong>of</strong> forces (3'<br />

= 0) ~q .(l3) becomes <strong>the</strong> geode-<br />

In <strong>the</strong> absence <strong>of</strong> matter, Eq. (14) is <strong>the</strong> same as in GRT.<br />

Thus, for instance, <strong>the</strong> questions discussed by Adler et aZ.7, Ser. 4.2,<br />

about space <strong>and</strong> time in a uniformly rotating system remain valid here.An<br />

interesting fact in this connection is that, on <strong>the</strong> one h<strong>and</strong>, space-time<br />

is flat in <strong>the</strong> rotating system (t,r,g,z), since curvature is an invariant.<br />

On <strong>the</strong> o<strong>the</strong>r h<strong>and</strong>, <strong>the</strong> 3-spatial geometry is curved. <strong>The</strong> reason is<br />

that <strong>the</strong> defini tion <strong>of</strong> distances dem<strong>and</strong>s <strong>the</strong> concept <strong>of</strong> s imu 1 tanei ty,<br />

<strong>and</strong> this is obtained by dt* = 0, where t* is a non-integrable time-coordina<br />

te 7 .<br />

For completeness, let us calculate <strong>the</strong> Gaussian curvature <strong>of</strong><br />

a plane z = const. in <strong>the</strong> rotating frame. <strong>The</strong> line element dk is given<br />

- 3~~ < O .<br />

(I- u2r2)<br />

We observe here that our <strong>the</strong>ory predicts a rotational red<br />

shift (see Ref.7, p.126), but no gravitational red shift, since gravity<br />

does not influence <strong>the</strong> metric. This is why we say that <strong>the</strong> <strong>the</strong>ory iscontradicted<br />

by experiment.

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