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56 ta ish

Ish: Kerr-Taub-NUT spacetime to explain the jet power and the radiative efficiency of astrophysical black holes

  1. Observables for bound orbital motion in axially symmetric space-times

    Eva Hackmann, Cláus Lämmerzahl

    Maqola20123 iqtibos
    ABI
  2. Gravomagnetic lensing by NUT space

    M. Nouri-Zonoz, D. Lynden–Bell

    Maqola19973 iqtibos
    ABI
  3. Dual-mass in general relativity

    Sriraṁ Ramaswamy, Amitabha Sen

    Maqola19812 iqtibos
    ABI
  4. The nut solution as a gravitational dyon

    J. S. Dowker

    Maqola19742 iqtibos
    ABI
  5. Global analysis of the Kerr-Taub-NUT metric

    John G. Miller

    Maqola19732 iqtibos
    ABI