Cosmic strings and the formation of galaxies and clusters of galaxies

Physics

Scientific paper

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Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

The evolution of density perturbations around cosmic strings in the matter-dominated era is discussed with attention to the specific nature of string perturbations. The parameter Gμ is calculated in two completely independent ways-from the requirements that Abell clusters are formed and that the galaxy-galaxy correlation function matches the observed one. Both values are consistent, lending support to the cosmic string theory.

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