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Exact Solution for the Exterior Field of a Rotating Neutron Star

Vladimir S. Manko·Eckehard W. Mielke·José D. Sanabria-Gómez
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Abstract

A four-parameter class of exact asymptotically flat solutions of the Einstein-Maxwell equations involving only rational functions is presented. It is able to describe the exterior field of a slowly or rapidly rotating neutron star with poloidal magnetic field.

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Vladimir S. Manko, Eckehard W. Mielke, José D. Sanabria-Gómez. 2000-01-25. Exact Solution for the Exterior Field of a Rotating Neutron Star. https://doi.org/10.1103/physrevd.61.081501

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