Figure 1 - uploaded by François R. Bouchet
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l/lOth of a 28& configuration after the universe has expanded by a fa+ tor of 2.25. The cube sides are equal to ct/2.
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The most fundamental issue in the theory of cosmic strings is addressed by means of Numerical Simulations: the existence of a scaling solution. The resolution of this question will determine whether cosmic strings can form the basis of an attractive theory of galaxy formation or prove to be a cosmological disaster like magnetic monopoles or domain...
