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- W1604317569 abstract "We discuss structure formation in cosmic string theories. Emphasis is laid on the properties of the peculiar velocity field, non-gaussian features and clusters of galaxies. It is found that the predicted peculiar velocity field is quiet ($v 30 h^{-1}$ Mpc) for models with ($Omega_0 h leq 0.2$) which is in disagreement with the results from POTENT at large scales ($>30h^{-1}$ Mpc), consistent, however, with the analysis of the peculiar velocity field of spiral galaxies by Giovannelli et al.. Using the Press-Schechter formalism we calculate the abundances of X-ray clusters. It is found that in CDM models a mass fluctuation $sigma_8 = 0.6...0.7$ is needed with $Omega_0 h =0.1...0.2$ in order to explain the current data." @default.
- W1604317569 created "2016-06-24" @default.
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- W1604317569 date "1998-10-26" @default.
- W1604317569 modified "2023-09-23" @default.
- W1604317569 title "Cosmic Strings and Structure Formation" @default.
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