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Approximation of the potential in scalar field dark energy models

Richard A. Battye and Francesco Pace*

  • Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom

  • *Corresponding author. francesco.pace@manchester.ac.uk
  • richard.battye@manchester.ac.uk

Phys. Rev. D 94, 063513 – Published 13 September, 2016

DOI: https://doi.org/10.1103/PhysRevD.94.063513

Abstract

We study the nature of potentials in scalar field based models for dark energy—with both canonical and noncanonical kinetic terms. We calculate numerically, and using an analytic approximation around a1, potentials for models with constant equation-of-state parameter wϕ. We find that for a wide range of models with canonical and noncanonical kinetic terms there is a simple approximation for the potential that holds when the scale factor is in the range 0.6a1.4. We discuss how this form of the potential can also be used to represent models with nonconstant wϕ and, hence, how it could be used in reconstruction from cosmological data.

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