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Prog. Theor. Phys. Vol. 70 No. 3 (1983) pp. 886-887

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Letters

Reduction of Partially Self-Similar Space-Times to Self-Similar Ones in General Relativity

Kenji Tomita and Robert T. Jantzen*

Research Institute for Theoretical Physics, Hiroshima University, Takehara, Hiroshima 725
*Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA

(Received June 13, 1983)

Abstract:

The definition of partially self-similar space-times introduced by one of the present authors is clarified and it is shown that compatibility with the Einstein equations reduced this class of space-times to the spatially self-similar case.


URL : http://ptp.ipap.jp/link?PTP/70/886/
DOI : 10.1143/PTP.70.886

[ Full Text PDF : FREE ACCESS (102K) ] Citation:


References:

  1. K. Tomita, Prog. Theor. Phys. 66 (1981), 2025[PTP].
  2. D. M. Eardley, Commun. Math. Phys. 37 (1974), 287[CrossRef].
  3. K. Tomita, Prog. Theor. Phys. Suppl. No. 70 (1981), 286[PTP].
  4. D. Eardley, E. Liang and R. Sachs, J. Math. Phys. 13 (1972), 99[CrossRef].
  5. J. W. York, Jr. in Sources of Gravitational Radiation, ed., L. Smarr (Cambridge University Press, Cambridge, 1979).
  6. R. T. Jantzen, Ann. of Phys. 127 (1980), 302[CrossRef].