New tests of the strong equivalence principle using binary-pulsar data

Physics

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Binary Stars, Gravitational Effects, Pulsars, Stellar Gravitation, Eccentricity, Gravitational Fields, Nonlinear Systems, Stellar Orbits

Scientific paper

One of the few experimental ways to investigate the nonlinear properties of the gravitational interaction is to test the 'strong equivalence principle', i.e., to test whether the ratio m(gravitational)/m(inertial) is 1 for self-gravitating bodies. It is pointed out that existing observational data on the class of small-eccentricity long-orbital-period binary pulsars already provide a limit which goes beyond the corresponding solar-system limits in probing strong-gravitational-field effects. Possible observational ways of improving this limit are suggested.

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