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Could thermal fluctuations seed cosmic structure?

✍ Scribed by Magueijo, João; Pogosian, Levon

Book ID
120008450
Publisher
The American Physical Society
Year
2003
Tongue
English
Weight
83 KB
Volume
67
Category
Article
ISSN
1550-7998

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## Abstract Intergalactic gravitational radiation fields with wavelengths in the range of 1 to 10^3^ Megaparsecs have remarkable observational effects if the energy density of the fields becomes comparable to the equivalent “critical” cosmological matter density χo = 3__H__~0~^2^. In this case the