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

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On Electromagnetic Thirr<strong>in</strong>g Problems 283<br />

the potentials <strong>in</strong> the exterior region read:<br />

In the region we set <strong>and</strong> The charge<br />

parameter should have the same value as <strong>in</strong> the exterior region because<br />

the shell at is uncharged. In or<strong>de</strong>r to enable cont<strong>in</strong>uous potentials<br />

<strong>and</strong> at the constant from (3 is generally different<br />

from 1, <strong>and</strong> a nontrivial time transformation is necessary <strong>in</strong> this<br />

region. Then the potentials <strong>in</strong> the region read:<br />

In the <strong>in</strong>terior region we have, due to <strong>and</strong><br />

<strong>and</strong> the potentials<br />

We now specify the parameter In our mo<strong>de</strong>ls, the function of<br />

the <strong>in</strong>ner shell is ma<strong>in</strong>ly to provi<strong>de</strong> a charge, <strong>and</strong> not so much to provi<strong>de</strong><br />

additional mass. It seems therefore reasonable to simplify our<br />

mo<strong>de</strong>ls (<strong>in</strong> accordance with [2, 3] by sett<strong>in</strong>g the rest mass <strong>de</strong>nsity of<br />

the <strong>in</strong>ner shell to zero. If we write E<strong>in</strong>ste<strong>in</strong>’s field equations <strong>in</strong> the<br />

form with be<strong>in</strong>g the electromagnetic energy–<br />

momentum tensor, then <strong>in</strong> our two–shell mo<strong>de</strong>ls consists of two parts:<br />

<strong>and</strong> <strong>and</strong> the are expressed by the<br />

<strong>de</strong>rivatives <strong>and</strong> <strong>in</strong> the form<br />

Equivalent relations are valid at the position With the useful<br />

abbreviations <strong>and</strong><br />

the condition leads to Herewith, the<br />

cont<strong>in</strong>uity conditions for <strong>and</strong> at <strong>and</strong> fix the<br />

constants as:

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