Effect of small-scale structure on the dynamics of cosmic strings

Physics

Scientific paper

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Scientific paper

The effective equation of state for a string with short-wavelength perturbations is shown to be μT=μ20, where μ and T are the mass density and tension in the rest frame of the string and μ0 is the unperturbed string tension. The dynamics of ``wiggly'' strings in flat spacetime is discussed. The conclusions are in agreement with the results obtained by Carter using different methods.

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