Abstract
Lukash and Novikov have given an interesting survey of their analyses of some of the features that may exist in the microwave background radiation in open universes. Here, we answer some criticisms that they make of our earlier analysis1, and point out a further unusual feature that appears in the temperature distribution of the most general flat and open cosmological models.
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References
Barrow, J. D., Juszkiewicz, R. & Sonoda, D. H. Nature 305, 397–402 (1983).
Barrow, J. D., Juszkiewicz, R. & Sonoda, D. H. Mon. Not. R. astr. Soc. 213, 917–943 (1985).
Collins, C. B. & Hawking, S. W. Mon. Not. R. astr. Soc. 162, 307–320 (1973).
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Barrow, J., Juszkiewicz, R. & Sonoda, D. Spottiness in the large-scale structure of the microwave background (reply). Nature 316, 48 (1985). https://doi.org/10.1038/316048a0
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DOI: https://doi.org/10.1038/316048a0
