Abstract
We consider the equilibrium configurations for static spherically symmetric self-gravitating perfect fluids in general relativity. The fluid obeys an equation of state which is the extreme limit allowed by Hawking's strong energy condition. The new solutions we have found are generalized Einstein static universes which have a Killing horizon similar to the one we are familiar with from the vacuum Schwarzschild solution.
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References
Penrose, R. (1965).Phys. Rev. Lett.,14, 57.
Hawking, S. W. (1966).Proc. R. Soc. (London),A295, 490.
Geroch, R. P. (1966).Phys. Rev. Lett.,17, 446.
Hawking, S. W., and Ellis, G. F. R. (1973).The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge).
The Zeldovich fluid which corresponds to aγ=2 equation of state has recently attracted attention for similar reasons.
Misner, C. W., Thorne, K. S., and Wheeler, J. A. (1973).Gravitation (W. H. Freeman and Company, San Francisco).
Plebanski, J. and Stachel, J. (1968).J. Math. Phys.,9, 269.
Geroch, R. P. (1969).Commun. Math. Phys.,13, 180.
Whittaker, E. T. (1935).Proc. R. Soc. (London),149, 384.
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Ibrahim, A., Nutku, Y. Generalized Einstein static universe. Gen Relat Gravit 7, 949–958 (1976). https://doi.org/10.1007/BF00766420
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DOI: https://doi.org/10.1007/BF00766420