External Electromagnetic Fields of a Slowly Rotating Magnetized Star with Nonvanishing Gravitomagnetic Charge

Details External Electromagnetic Fields of a Slowly Rotating Magnetized Star with Nonvanishing Gravitomagnetic Charge External Electromagnetic Fields of a Slowly Rotating Magnetized Star with Nonvanishing Gravitomagnetic Charge

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.2098a&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

We write Maxwell equations in the external background spacetime of a slowly rotating magnetized NUT star and find analytical solutions after separating them into angular and radial parts. The star is considered isolated and in vacuum, with monopolar configuration model for the stellar magnetic field. The contribution to the external field from the NUT charge and frame-dragging effect are considered in detail.

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