Primordial Origin of Nontopological Solitons

Joshua A. Frieman, Graciela B. Gelmini, Marcelo Gleiser, and Edward W. Kolb
Phys. Rev. Lett. 60, 2101 – Published 23 May 1988
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Abstract

We discuss the formation of nontopological solitons in a second-order phase transition in the early Universe. Ratios of dimensionless coupling constants in the Lagrangean determine their abundance and mass. For a large range of parameters, nontopological solitons can be cosmologically significant, contributing a significant fraction of the present mass density of the Universe.

  • Received 20 January 1988

DOI:https://doi.org/10.1103/PhysRevLett.60.2101

©1988 American Physical Society

Authors & Affiliations

Joshua A. Frieman1, Graciela B. Gelmini2, Marcelo Gleiser3, and Edward W. Kolb3

  • 1Stanford Linear Accelerator Center, Stanford University, Stanford, California 94305
  • 2International Center for Theoretical Physics, and International School for Advanced Studies, 34100 Trieste, Italy
  • 3NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510

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Vol. 60, Iss. 21 — 23 May 1988

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