Charge, geometry, and effective mass in the Kerr-Newman solution to the Einstein field equations

Details Charge, geometry, and effective mass in the Kerr-Newman solution to the Einstein field equations Charge, geometry, and effective mass in the Kerr-Newman solution to the Einstein field equations

2008-05-09

arxiv.org/abs/0805.1417v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

To appear in Foundations of Physics. Misprints have been corrected. 14 pages, 4 figures

Scientific paper

10.1007/s10701-008-9245-x

It has been shown that for the Reissner-Nordstrom solution to the vacuum
Einstein field equations charge, like mass, has a unique space-time signature
[Found. Phys. 38, 293-300 (2008)]. The presence of charge results in a negative
curvature. This work, which includes a discussion of effective mass, is
extended here to the Kerr-Newman solution.

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