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

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

tric potential there is no electric field. That means that another<br />

metallic sphere <strong>in</strong>si<strong>de</strong> the sphere of potential should have the same<br />

potential. This is only possible if the potential for a charged po<strong>in</strong>t particle<br />

has the form that is, if the potential is a harmonic function. If<br />

the equation, namely the Poisson equation which <strong>de</strong>term<strong>in</strong>es<br />

the potential from the charge distribution <strong>and</strong> the boundary conditions,<br />

has a different form, then the solution is different from <strong>and</strong> does not<br />

show up this property.<br />

The most recent experiment of this k<strong>in</strong>d has been carried through by<br />

Williams, Faller, <strong>and</strong> Hill [23]. Until now, the theoretical <strong>in</strong>terpretation<br />

of this k<strong>in</strong>d is experiments is restricted to three mo<strong>de</strong>ls only, namely (i)<br />

to the mo<strong>de</strong>l of a scalar photon mass see [23, 24] <strong>and</strong> references<br />

there<strong>in</strong>, which gives a potential of the form<br />

(ii) to a specific ansatz for a <strong>de</strong>viation from the Coulomb law,<br />

<strong>and</strong> (iii) to the context of a vector valued photon mass [25]. No<br />

<strong>de</strong>viation from Coulomb’s law has been found <strong>and</strong> from the accuracy<br />

of the apparatus one gets the estimates or<br />

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

Behaviour of atomic clocks. Any modification of the solution for<br />

the potential of a po<strong>in</strong>t charge should modify the properties of atoms, especially<br />

the energy eigenvalues. As a consequence, the Rydberg constant<br />

will be modified. Not much has been calculated <strong>in</strong> that context. The<br />

modification for a pure Yukawa modification of the Coulomb potential<br />

(20) leads to modified transition frequencies. If one compares a transition<br />

for small quantum numbers, <strong>and</strong> large quantum numbers N,<br />

M, then the Rydberg constant may be different, s<strong>in</strong>ce the strength of<br />

the electric field near the atomic core is different from the strength far<br />

from it. This difference is calculated to be [26]<br />

where is Bohr’s radius. From correspond<strong>in</strong>g spectroscopic experiments<br />

one <strong>de</strong>rives for<br />

4.4. TESTS OF SPECIAL RELATIVITY<br />

The ma<strong>in</strong> experiments for Special Relativity test the constancy of the<br />

speed of light: Michelson–Morley–experiments [13, 14] test the direc-

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