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

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60 EXACT SOLUTIONS AND SCALAR FIELDS IN GRAVITY<br />

not vanish <strong>in</strong> the stationary solution (27). In any case rotational effects<br />

are responsible for balanc<strong>in</strong>g the gravitational attraction such that<br />

time–<strong>in</strong><strong>de</strong>pen<strong>de</strong>nt configurations can exist at all <strong>and</strong> mutual focus<strong>in</strong>g<br />

does not occur.<br />

The <strong>de</strong>rivation of the exact null fluid solutions (18) <strong>and</strong> (27) was<br />

first given <strong>in</strong> our paper [7]. For a discussion <strong>and</strong> illustration of the<br />

trajectories (screwed motion), see [9]. There<strong>in</strong> Fermi coord<strong>in</strong>ates along<br />

the world l<strong>in</strong>e of a fixed po<strong>in</strong>t on the cyl<strong>in</strong><strong>de</strong>r mantle are <strong>in</strong>troduced to<br />

confirm the <strong>in</strong>terpretation of the photon trajectories.<br />

3.4. OTHER SOLUTIONS<br />

We have mentioned that the quantity S <strong>de</strong>f<strong>in</strong>ed <strong>in</strong> (14) factorizes for<br />

K = U. This holds also for the special choice K = –2U. In both cases<br />

one can put either of the two factors <strong>in</strong> S equal to zero. In this way<br />

one obta<strong>in</strong>s four different static solutions which are listed <strong>in</strong> [8]. The<br />

result<strong>in</strong>g mass <strong>de</strong>nsity profiles plotted <strong>in</strong> [8] are well-behaved only <strong>in</strong> the<br />

solution treated here.<br />

The attempt to start with a metric admitt<strong>in</strong>g an Abelian group<br />

where none of the Kill<strong>in</strong>g vectors is hypersurface–orthogonal did not<br />

lead to more general solutions. The existence of three twist<strong>in</strong>g Kill<strong>in</strong>g<br />

vectors is not compatible with the structure (13) of the propagation<br />

vectors. Hence there are only two possibilities: the non–twist<strong>in</strong>g Kill<strong>in</strong>g<br />

vector is either timelike or spacelike, i.e. the gravitational field is either<br />

static or stationary <strong>and</strong> the correspond<strong>in</strong>g metrics are (12) <strong>and</strong> (27),<br />

respectively.<br />

One can <strong>in</strong>terchange the coord<strong>in</strong>ates <strong>and</strong> <strong>in</strong> the static solution<br />

(18) to obta<strong>in</strong> a metric for counter–rotat<strong>in</strong>g null dust components, but<br />

then the axis is not regular.<br />

4. DISCUSSION<br />

Un<strong>de</strong>r certa<strong>in</strong> conditions the superposition of two null dust components<br />

propagat<strong>in</strong>g <strong>in</strong> opposite spatial directions gives rise to static (or<br />

stationary) gravitational fields <strong>in</strong> the <strong>in</strong>teraction region. Examples consi<strong>de</strong>red<br />

<strong>in</strong> this article are the static spherically symmetric solution (10)<br />

<strong>de</strong>rived <strong>in</strong> [6], the static cyl<strong>in</strong>drically symmetric solution (18) <strong>de</strong>rived <strong>in</strong><br />

[7], <strong>and</strong> its stationary counterpart (27). These three metrics are given<br />

<strong>in</strong> closed form by <strong>in</strong>troduc<strong>in</strong>g suitable coord<strong>in</strong>ates.<br />

The superposition of counter–mov<strong>in</strong>g pencils of light implies a rotational<br />

effect which compensates for the gravitational attraction to prevent<br />

mutual focus<strong>in</strong>g of the rays. An important po<strong>in</strong>t is the fact that<br />

the propagation null vectors of the two null dust components are both

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