Large-scale structure from wiggly cosmic strings

Tanmay Vachaspati and Alexander Vilenkin
Phys. Rev. Lett. 67, 1057 – Published 26 August 1991
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Abstract

Recent simulations of the evolution of cosmic strings indicate the presence of small-scale structure on the strings. We show that wakes produced by such ‘‘wiggly’’ cosmic strings can result in the efficient formation of large-scale structure and large streaming velocities in the Universe without significantly affecting the microwave-background isotropy. We also argue that the motion of strings will lead to the generation of a primordial magnetic field. The most promising version of this scenario appears to be the one in which the Universe is dominated by light neutrinos.

  • Received 7 March 1991

DOI:https://doi.org/10.1103/PhysRevLett.67.1057

©1991 American Physical Society

Authors & Affiliations

Tanmay Vachaspati and Alexander Vilenkin

  • Tufts Institute of Cosmology, Department of Physics and Astronomy, Tufts University, Medford, Massachusetts 02155

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Issue

Vol. 67, Iss. 9 — 26 August 1991

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