Constraining the electric charges of some astronomical bodies in
Reissner-Nordstrom spacetimes and generic r^-2-type power-law potentials from
orbital motions [PDF]
Lorenzo IorioWe put model-independent, dynamical constraints on the net electric charge Q of some astronomical and astrophysical objects by assuming that their exterior spacetimes are described by the Reissner-Nordstroem metric, which induces an additional potential U_RN \propto Q^2 r^-2. Our results extend to other hypothetical power-law interactions inducing extra-potentials U_pert = r^-2 as well (abridged).View original: http://arxiv.org/abs/1112.3520
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