Limiting Braneworlds with the Binary Pulsar

Physics

Scientific paper

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Scientific paper

In this paper we calculate the emission of gravity waves by the binary pulsar in the framework of five dimensional braneworlds. We consider only braneworlds with one compact extra-dimension. We show that the presence of additional degrees of freedom, especially the `gravi-scalar' leads to a modification of Einstein's quadrupole formula. We compute the induced change for the binary pulsar PSR 1913+16 in the simple example of a 5d Minkowski background. It amounts to about 20% which is by far excluded by present experimental data.

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