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Exact Solutions and Scalar Fields in Gravity - Instituto Avanzado de ...

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312<br />

First let us recall some properties of the Gö<strong>de</strong>l metric [9] which is of<br />

great importance <strong>in</strong> construct<strong>in</strong>g several types of exact LFFS. For the<br />

signature (+ – – –) <strong>and</strong> after some other transformations, the Gö<strong>de</strong>l<br />

metric reads (cf. [22, 24])<br />

or <strong>in</strong> “cyl<strong>in</strong>drical” coord<strong>in</strong>ates,<br />

the same form <strong>in</strong> [20] was put as<br />

EXACT SOLUTIONS AND SCALAR FIELDS IN GRAVITY<br />

It is <strong>in</strong>terest<strong>in</strong>g that if (1) is rewritten <strong>in</strong> the form<br />

it becomes clear that either of <strong>and</strong> may be <strong>in</strong>terpreted as a time<br />

coord<strong>in</strong>ate (obviously related to the existence of closed timelike l<strong>in</strong>es <strong>in</strong><br />

the Gö<strong>de</strong>l universe). Then, <strong>in</strong>terchang<strong>in</strong>g <strong>and</strong> <strong>in</strong> this expression, we<br />

get<br />

(the three–dimensional sector tak<strong>in</strong>g here the Cartesian form). Of course,<br />

all coord<strong>in</strong>ates used above are, as it is admitted traditionally <strong>in</strong> the<br />

Gö<strong>de</strong>l metric, dimensionless. One can however <strong>in</strong>corporate <strong>in</strong>to (at<br />

least, some) coord<strong>in</strong>ates variables <strong>and</strong> re<strong>de</strong>f<strong>in</strong>e so that,<br />

for example, (1) takes the form<br />

then the limit yields the M<strong>in</strong>kowski spacetime.<br />

The Gö<strong>de</strong>l spacetime admits five Kill<strong>in</strong>g vectors which we give here<br />

<strong>in</strong> the coord<strong>in</strong>ates used <strong>in</strong> (2), up to the positive constant factor<br />

occurr<strong>in</strong>g <strong>in</strong> the covariant components:

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