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

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

field has here to be of purely magnetic type, hav<strong>in</strong>g the mean<strong>in</strong>g of the<br />

(constant) proper magnetic field <strong>in</strong>tensity. Then it is natural to assume<br />

so that <strong>and</strong><br />

There are only two natural approaches to solve the problem un<strong>de</strong>r<br />

consi<strong>de</strong>ration: either (i) one may choose the behaviour of <strong>and</strong> f<strong>in</strong>d<br />

via straightforward <strong>in</strong>tegration of (19), or (ii) postulate the velocity<br />

distribution <strong>and</strong> f<strong>in</strong>d merely by a differentiation. Thus our task<br />

proves to be a trivial one. The general properties of the fluid now are<br />

formulated as follows: Its particles are mov<strong>in</strong>g <strong>in</strong>ertially (the velocity is<br />

constant <strong>in</strong> the direction of motion though it <strong>de</strong>pends on the concrete<br />

layer, thus be<strong>in</strong>g a function of only); if the velocity vanishes on two<br />

opposite boundaries, the charge <strong>de</strong>nsity nearby has to take opposite<br />

signs; f<strong>in</strong>ally, the constant proper magnetic field is directed along axis.<br />

As illustrations, we just mention four special solutions:<br />

1.<br />

2. when e.g.,<br />

Then,<br />

3. now,<br />

4. The next special case meets the follow<strong>in</strong>g alternative condition:<br />

This solution can be easily jo<strong>in</strong>ed with a constant sourceless magnetic<br />

field (the exterior solution) at one or two (not necessarily consecutive)<br />

no<strong>de</strong>s.<br />

4. CONCLUSIONS<br />

We have shown <strong>in</strong> this communication that LFFS exist not only <strong>in</strong><br />

general relativity, but also <strong>in</strong> flat spacetimes <strong>and</strong> even <strong>in</strong> the case when<br />

charged fluids are nonrelativistic. These latter cases are of importance<br />

s<strong>in</strong>ce then a superposition of electromagnetic fields is applicable (the<br />

Maxwell theory is completely l<strong>in</strong>ear, <strong>and</strong> there is no self–<strong>in</strong>teraction of<br />

electromagnetic fields due to their contribution to curvature characteristic<br />

for general relativity). In these flat–spacetime solutions the Lorentz<br />

force is compensated by <strong>in</strong>fluence of a source–free (usually, purely magnetic)<br />

field. Our <strong>in</strong>terpretation of the general relativistic LFFS is that<br />

they should conta<strong>in</strong> these source–free electromagnetic part which cannot<br />

be separated from that created by charged fluid proper <strong>in</strong> the nonl<strong>in</strong>ear<br />

realm of general relativity. Even an overcompensation of the Lorentz

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