Exact Solution for the Exterior Field of a Rotating Neutron Star
arXiv:gr-qc/0001081 · doi:10.1103/PhysRevD.61.081501
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.
Accepted for publication in Phys. Rev. D as Rapid Communication. 8 pages, 2 eps figures
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