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Microwave anisotropies from texture seeded structure formation

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Microwave anisotropies from texture seeded structure formation

DURRER, Ruth, HOWARD, Armando, ZHOU, Zhi-Hong

Abstract

The microwave anisotropy in a scenario of large scale structure formation with cold dark matter and texture is discussed. The authors find that in this scenario small scale fluctuations (on angular scales of a few degrees and less) are very effectively damped by photon diffussion. On a scale of 10 - 20 degrees they predict peaks with ampliutdes of ΔT/T ≍ (1 - 5)×10-5. About 5 to 10 such peaks are expected all over the sky. This result tells us that texture seeded structure formation is likely to be ruled out (or confirmed!) within the near future.

DURRER, Ruth, HOWARD, Armando, ZHOU, Zhi-Hong. Microwave anisotropies from texture seeded structure formation. Physical Review. D , 1994, vol. 49, p. 681-691

DOI : 10.1103/PhysRevD.49.681 arxiv : astro-ph/9311040

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http://archive-ouverte.unige.ch/unige:992

Disclaimer: layout of this document may differ from the published version.

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