Physics
Scientific paper
Apr 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..33.2175t&link_type=abstract
Physical Review D (Particles and Fields), Volume 33, Issue 8, 15 April 1986, pp.2175-2181
Physics
170
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.
Brandenberger Robert H.
Turok Neil
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