Stationary Line of N Kerr Masses Kept Apart by Gravitational Spin-Spin Interaction

Details Stationary Line of N Kerr Masses Kept Apart by Gravitational Spin-Spin Interaction Stationary Line of N Kerr Masses Kept Apart by Gravitational Spin-Spin Interaction

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phrvl..50.1027y&link_type=abstract

Physical Review Letters, Volume 50, Issue 14, April 4, 1983, pp.1027-1030

Physics

18

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Scientific paper

The metric is presented, in terms of six determinants of degree N, in a concise closed form, describing N collinear isolated Kerr masses (N=1, 2, 3, ...) balanced by their gravitational spin-spin interaction. Two hitherto unnoticed potentials L and M are introduced to evaluate the metric function ω. The conditions for regularity of the metric on the symmetrical axis are presented.

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