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Spontaneous generation of density perturbations in the early Universe

Nature volume 298, pages 538–540 (1982)Cite this article

Abstract

A long-standing problem in cosmology has been to understand the origins of density inhomogeneities in the Universe. Calculations involving inhomogeneities have for the most part required the assumption of some initial spectrum of perturbations, which is inserted ‘by hand’. We present here a mechanism for the spontaneous creation of density perturbations during the transition in the early Universe from unconfined quark matter to hadronic matter. The subsequent evolution of these perturbations remains a problem for further study.

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Authors and Affiliations

  1. Astronomy and Astrophysics Center, The University of Chicago, Chicago, Illinois, 60637, USA

    Matt Crawford & David N. Schramm

Authors
  1. Matt Crawford
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  2. David N. Schramm
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Crawford, M., Schramm, D. Spontaneous generation of density perturbations in the early Universe. Nature 298, 538–540 (1982). https://doi.org/10.1038/298538a0

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