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

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

<strong>and</strong> one <strong>in</strong>homogeneous Maxwell equation<br />

Eq. (20) together with enforces the ansatz<br />

with a dimensionless function Eq. (21) then results<br />

<strong>in</strong> the form with These forms<br />

constitute the dipole character of the (rotationally <strong>in</strong>duced) magnetic<br />

field. Eqs. (20) <strong>and</strong> (22) constitute two coupled ord<strong>in</strong>ary differential<br />

equations for the functions <strong>and</strong> In the <strong>in</strong>terior these<br />

equations simplify drastically, <strong>and</strong> give the results<br />

with dimensionless constants <strong>and</strong> i.e. the <strong>in</strong>terior stays flat, <strong>and</strong><br />

the magnetic field has (<strong>in</strong> Cartesian coord<strong>in</strong>ates) only a (constant)<br />

In the <strong>in</strong>termediate <strong>and</strong> exterior regions, due to<br />

one <strong>in</strong>tegration of Eq. (20) is trivial:<br />

with a dimensionless <strong>in</strong>tegration constant Insertion of (23) <strong>in</strong>to (22),<br />

together with outsi<strong>de</strong> the charged shell, results <strong>in</strong><br />

The general solution of Eq. (25) has the form<br />

with dimensionless <strong>in</strong>tegration constants <strong>and</strong> <strong>and</strong> where<br />

is a special <strong>in</strong>homogeneous solution, <strong>and</strong> are <strong>in</strong><strong>de</strong>pen<strong>de</strong>nt<br />

homogeneous solutions of (24). Luckily, there exist simple polynomial<br />

solutions<br />

<strong>and</strong> can then be found from by d’Alembert’s reduction procedure:<br />

with

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