Density Fluctuations from Strings and Galaxy Formation

Alexander Vilenkin and Qaisar Shafi
Phys. Rev. Lett. 51, 1716 – Published 31 October 1983
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Abstract

The spectra of density fluctuations caused by strings in a universe dominated either by baryons, neutrinos, or axions are presented. Realistic scenarios for galaxy formation seem possible in all three cases. Examples of grand unified theories which lead to strings with the desired mass scales are given.

  • Received 20 June 1983

DOI:https://doi.org/10.1103/PhysRevLett.51.1716

©1983 American Physical Society

Authors & Affiliations

Alexander Vilenkin

  • Physics Department, Tufts University, Medford, Massachusetts 02155

Qaisar Shafi*

  • National Aeronautics and Space Administration Goddard Space Flight Center, Greenbelt, Maryland 20771, and International Center for Theoretical Physics, Trieste, Italy

  • *Present address: Bartol Institute, University of Delaware, Newark, Del. 19711.

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Issue

Vol. 51, Iss. 18 — 31 October 1983

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