Exact Solution for the Exterior Field of a Rotating Neutron Star

Details Exact Solution for the Exterior Field of a Rotating Neutron Star Exact Solution for the Exterior Field of a Rotating Neutron Star

2000-01-25

arxiv.org/abs/gr-qc/0001081v1

Phys.Rev.D61:081501,2000

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Accepted for publication in Phys. Rev. D as Rapid Communication. 8 pages, 2 eps figures

Scientific paper

10.1103/PhysRevD.61.081501

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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