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Pressureless disk cannot be the source for the Kerr metric

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Lettere al Nuovo Cimento (1971-1985)

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References

  1. B. Carter:Black-hole equilibrium states, inBlack Holes, edited byC. DeWitt andB. S. DeWitt (New York, N. Y., 1973).

  2. J. M. Bardeen:Rapidity rotating stars, disks and black holes, inBlack Holes, edited byC. DeWitt andB. S. DeWitt (New York, N. Y., 1973).

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Author notes

  1. M. A. Abramowicz, W. Arkuszewski & B. Muchotrzeb

    Present address: Institute of Astronomy, Polish Academy of Sciences, Warszawa, Poland

Authors and Affiliations

  1. Institute of Theoretical Physics, Department of Physics, Stanford University, 94305, Stanford, Cal.

    M. A. Abramowicz

Authors
  1. M. A. Abramowicz
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  2. W. Arkuszewski
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  3. B. Muchotrzeb
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Additional information

Work supported in part by U.S. National Science Foundation, grant MPS 74-15524.

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Abramowicz, M.A., Arkuszewski, W. & Muchotrzeb, B. Pressureless disk cannot be the source for the Kerr metric. Lett. Nuovo Cimento 15, 477–479 (1976). https://doi.org/10.1007/BF02725151

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  • DOI: https://doi.org/10.1007/BF02725151

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