Abstract
The elliptic boundary value problem governing the steady electrical heating of a conductor of heat and electricity, the so-called thermistor problem,
where \({\sigma }(u)\) is the temperature dependent electric conductivity and \({\kappa }(u)\) the thermal conductivity, admits a reinterpretation in the framework of general relativity if we choose \({\sigma }(u)=e^u\), \({\kappa }(u)=1\) and, in addition, \({\Omega }\) is a domain of \({\mathbf{R}^3}\) axially symmetric whereas the function \(\phi _b\), in a cylindrical coordinate system \({\rho },z,{\varphi }\), is independent of \({\varphi }\). The same analytical methods relevant in the thermistor problem can be used in this new context.
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Notes
In the Einstein equations we assume \(\frac{k}{c^4}=1\) (k gravitational constant).
The semicolon denotes the covariant differentiation.
A physically realistic situation could be to assume the boundary of \({\Omega }\) divided into two disjoint parts \({\Gamma }_1\) and \({\Gamma }_2\) representing the electrodes of the device.
This assumption is not restrictive since the electric potential \(\phi \) is defined apart an arbitrary constant.
If the two constants are equal the problem has only the trivial solution.
This is of course the key point, see for the proof [5].
Note that \(\Psi (\phi )\) can be written down explicitly.
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Cimatti, G. A nonlinear elliptic boundary value problem relevant in general relativity and in the theory of electrical heating of conductors. Boll Unione Mat Ital 11, 191–204 (2018). https://doi.org/10.1007/s40574-017-0121-5
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DOI: https://doi.org/10.1007/s40574-017-0121-5
Keywords
- Axially symmetric gravitational fields
- Existence and uniqueness of solutions
- Weyl–Lewis–Papapetrou coordinates