Light-cone cuts of I(+) for charged-Kerr geometry

Details Light-cone cuts of I(+) for charged-Kerr geometry Light-cone cuts of I(+) for charged-Kerr geometry

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984gregr..16.1157j&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 16, Dec. 1984, p. 1157-1162.

Computer Science

1

Infinity, Kerr Effects, Light-Cone Expansion, Relativity, Space-Time Functions, Geodesic Lines, Integral Equations

Scientific paper

The light-cone cut function (Z) of future null infinity I(+) introduced by Joshi et al. (1983) and Kozameh and Newman (1983) as a nonlocal variable to study asymptotically flat space-times in general relativity is applied to charged Kerr metrics. The equations for null geodesics are integrated, and Z is obtained parametrically as three equations involving elliptical integrals. The complexity of the cut function is attributed to the nonvanishing mass, charges, and angular momentum, as in the Schwarzschild case studied by Joshi et al. (1983).

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