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We study the structure of electromagnetic field of slowly rotating magnetizedstar in a Randall-Sundrum II type braneworld. The star is modeled as a sphereconsisting of perfect highly magnetized fluid with infinite conductivity andfrozen-in dipolar magnetic field. Maxwell's equations for the external magneticfield of the star in the braneworld are analytically solved in approximation ofsmall distance from the surface of the star. We have also found numericalsolution for the electric field outside the rotating magnetized neutron star inthe braneworld in dependence on brane tension. The influence of brane tensionon the electromagnetic energy losses of the rotating magnetized star isunderlined. Obtained "brane" corrections are shown to be relevant and havenon-negligible values. In comparison with astrophysical observations on pulsarsspindown data they may provide an evidence for the brane tension and, thus,serve as a test for the braneworld model of the Universe.

Electromagnetic Fields of Slowly Rotating Compact Magnetized Stars in Braneworld