skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The stochastic spectator

Journal Article · · Journal of Cosmology and Astroparticle Physics
; ;  [1]; ;  [2]
  1. Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth, PO1 3FX (United Kingdom)
  2. Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH (United Kingdom)

We study the stochastic distribution of spectator fields predicted in different slow-roll inflation backgrounds. Spectator fields have a negligible energy density during inflation but may play an important dynamical role later, even giving rise to primordial density perturbations within our observational horizon today. During de-Sitter expansion there is an equilibrium solution for the spectator field which is often used to estimate the stochastic distribution during slow-roll inflation. However slow roll only requires that the Hubble rate varies slowly compared to the Hubble time, while the time taken for the stochastic distribution to evolve to the de-Sitter equilibrium solution can be much longer than a Hubble time. We study both chaotic (monomial) and plateau inflaton potentials, with quadratic, quartic and axionic spectator fields. We give an adiabaticity condition for the spectator field distribution to relax to the de-Sitter equilibrium, and find that the de-Sitter approximation is never a reliable estimate for the typical distribution at the end of inflation for a quadratic spectator during monomial inflation. The existence of an adiabatic regime at early times can erase the dependence on initial conditions of the final distribution of field values. In these cases, spectator fields acquire sub-Planckian expectation values. Otherwise spectator fields may acquire much larger field displacements than suggested by the de-Sitter equilibrium solution. We quantify the information about initial conditions that can be obtained from the final field distribution. Our results may have important consequences for the viability of spectator models for the origin of structure, such as the simplest curvaton models.

OSTI ID:
22667648
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2017, Issue 10; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Spectator field dynamics in de Sitter and curvaton initial conditions
Journal Article · Mon Oct 01 00:00:00 EDT 2012 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22667648

Stochastic inflation revisited: non-slow-roll statistics and DBI inflation
Journal Article · Tue Apr 15 00:00:00 EDT 2008 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22667648

Planck 2013 results. XXII. Constraints on inflation
Journal Article · Wed Oct 29 00:00:00 EDT 2014 · Astronomy and Astrophysics · OSTI ID:22667648