Cosmology with a primordial scaling field

Pedro G. Ferreira and Michael Joyce
Phys. Rev. D 58, 023503 – Published 9 June 1998
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Abstract

A weakly coupled scalar field Φ with a simple exponential potential V=MP4exp(λΦ/MP) where MP is the reduced Planck mass, and λ>2, has an attractor solution in a radiation or matter dominated universe in which it mimics the scaling of the dominant component, contributing a fixed fraction Ωφ (determined by λ) to the energy density. Such fields arise generically in particle physics theories involving compactified dimensions, with values of λ which give a cosmologically relevant Ωφ. For natural initial conditions on the scalar field in the early universe the attractor solution is established long before the epoch of structure formation, and in contrast with the solutions used in other scalar field cosmologies, it is one which does not involve an energy scale for the scalar field characteristic of late times. We study in some detail the evolution of matter and radiation perturbations in a standard inflation-motivated Ω=1 dark-matter dominated cosmology with this extra field. Using a full Einstein-Boltzmann calculation we compare observable quantities with current data. We find that, for Ωφ0.080.12, these models are consistent with large angle cosmic microwave background anisotropies as detected by COBE, the linear mass variance as compiled from galaxy surveys, big bang nucleosynthesis, the abundance of rich clusters and constraints from the Lyman-α systems at high redshift. Given the simplicity of the model, its theoretical motivation and its success in matching observations, we argue that it should be taken on a par with other currently viable models of structure formation.

  • Received 11 November 1997

DOI:https://doi.org/10.1103/PhysRevD.58.023503

©1998 American Physical Society

Authors & Affiliations

Pedro G. Ferreira

  • Center for Particle Astrophysics, 301 Leconte Hall, University of California, Berkeley, California 94720

Michael Joyce

  • School of Mathematics, Trinity College, Dublin 2, Ireland

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Vol. 58, Iss. 2 — 15 July 1998

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