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Example 1.
For our first example we use the standard metric on the sphere.
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| (2.2) |
Define a unit vector field .
M >
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| (2.3) |
We see that the congruence is geodesic on the equator () but is accelerating elsewhere. It is shearing, rotating and non-expanding.
M >
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| (2.4) |
Example 2.
For the next example we consider a class of Robinson-Trautman metrics. These are of Petrov type II and admit a null congruence which is shear-free.
M >
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RT >
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| (2.6) |
Here is a null tetrad for this metric.
RT >
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| (2.7) |
The null congruence is very simple:
| (2.8) |
First calling sequence:
RT >
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| (2.9) |
Third calling sequence:
RT >
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| (2.10) |
Fourth calling sequence
RT >
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| (2.11) |
Example 3.
Here is an example of a Newman-Tamburino metric of Petrov type I and which admits a null geodesic congruence with non-vanishing shear.
RT >
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M >
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| (2.13) |
Here is a null tetrad for this metric.
M >
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| (2.14) |
Again we consider the first leg of this tetrad.
| (2.15) |
First calling sequence:
RT >
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| (2.16) |
Third calling sequence:
RT >
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| (2.17) |
Fourth calling sequence:
RT >
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| (2.18) |