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Prog. Theor. Phys. Vol. 70 No. 3 (1983) pp. 886-887
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
References:
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D. M. Eardley, Commun. Math. Phys. 37 (1974), 287[CrossRef].
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D. Eardley, E. Liang and R. Sachs, J. Math. Phys. 13 (1972), 99[CrossRef].
- J. W. York, Jr. in Sources of Gravitational Radiation, ed., L. Smarr (Cambridge University Press, Cambridge, 1979).
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R. T. Jantzen, Ann. of Phys. 127 (1980), 302[CrossRef].