English

Fully Electrified Neugebauer Spacetimes

General Relativity and Quantum Cosmology 2009-10-22 v2

Abstract

Generalizing a method presented in an earlier paper, we express the complex potentials E and Phi of all stationary axisymmetric electrovac spacetimes that correspond to axis data of the form E(z,0) = (U-W)/(U+W) , Phi(z,0) = V/(U+W) , where U = z^{2} + U_{1} z + U_{2} , V = V_{1} z + V_{2} , W = W_{1} z + W_{2} , in terms of the complex parameters U_{1}, V_{1}, W_{1}, U_{2}, V_{2} and W_{2}, that are directly associated with the various multipole moments. (Revised to clarify certain subtle points.)

Cite

@article{arxiv.gr-qc/9407027,
  title  = {Fully Electrified Neugebauer Spacetimes},
  author = {Frederick J. Ernst},
  journal= {arXiv preprint arXiv:gr-qc/9407027},
  year   = {2009}
}

Comments

25 pages, REVTEX

R2 v1 2026-07-22T12:49:21.793Z