Abstract
We point out that the conclusions of a recent Letter by Yavuzet al. are based on a misunderstanding of basic perturbation theory.
References
Bayin, S. S.: 1983,Phys. Rev. D27, 3030.
Bayin, S. S.: 1985a,Phys. Rev. D32, 2241.
Bayin, S. S.: 1985b,Can. J. Phys. 63, 1320.
Bayin, S. S.: 1989,Astrophys. Space Sci. 161, 351.
Bayin, S. S. and Cooperstock, F. I.: 1980,Phys. Rev. D22, 2317.
Cohen, J. M.: 1971, in Davies and Smith (eds.),Crab Nebula, p. 334.
Hartle, J. B.: 1967,Astrophys. J. 150, 1005.
Krori, K. D., Sarmah, J. C., and Gaswami, D.: 1983,Can. J. Phys. 61, 744.
Lausberg, A.: 1980,Astron. Astrophys. 82, 1.
Stewart, B. W.: 1983,J. Phys. 16, 1689.
Whitman, P. G.: 1982,Phys. Letters 89A, 129.
Yavuz, I., Battal, C., and Baysal, H.: 1990,Astrophys. Space Sci. 167, 341.
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Bayin, S.S. Reply to I. Yavuz, C. Battal, and H. Baysal on slow rotational perturbations of Friedmann universes. Astrophys Space Sci 187, 147–148 (1992). https://doi.org/10.1007/BF00642696
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DOI: https://doi.org/10.1007/BF00642696