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WIGGLY STRINGS OF RADIAL CONFIGURATION IN THE KERR BLACK HOLE

    https://doi.org/10.1142/S0217732311036425Cited by:1 (Source: Crossref)

    Previously we investigated classical motion of a string in (3+1)-dimensional spherically symmetric neutral and charged black holes. As an extension the solutions in (3+1)-dimensional axially symmetric rotating black hole are investigated. The solutions for the wiggly string exhibit open strings lying in the radial direction in the equatorial plane outside the horizon.