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Decreasing density perturbations and the isotropy of the cosmic microwave background

Флуктуации убывающей плотности и изотропия космического микроволнового фона

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Il Nuovo Cimento B (1971-1996)

Summary

We compute the effect on the small-scale anisotropy of the cosmic background radiation induced by decreasing density fluctuations in a spatially flat Robertson-Walker universe.

Riassunto

Si calcola l’effetto sull'isotropia della, radiazione cosmica di fondo indotto da fluttuazioni di densità decrescenti in un universo di Robertson-Walker spazialmente piatto.

Резюме

Мы определясм влияние на изотропию космического излучения фона флуктуаций убываущей плотности в пространственно плоской вселенной Робертсона-Уолкера.

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Authors and Affiliations

  1. Dipartimento di Matematica dell’Università, Catania

    S. Motta

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  1. S. Motta
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Motta, S. Decreasing density perturbations and the isotropy of the cosmic microwave background. Nuov Cim B 102, 517–522 (1988). https://doi.org/10.1007/BF02728783

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  • DOI: https://doi.org/10.1007/BF02728783

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