Please use this identifier to cite or link to this item: http://hdl.handle.net/10773/24029
Title: The role of fluctuation-dissipation dynamics in setting initial conditions for inflation
Author: Bastero-Gil, Mar
Berera, Arjun
Brandenberger, Robert
Ramos, Rudnei O.
Rosa, João G.
Moss, Ian G.
Keywords: Inflation
Initial conditions and eternal universe
Particle physics - cosmology connection
Physics of the early universe
Issue Date: 2018
Publisher: IOP Publishing
Abstract: We study the problem of initial conditions for slow-roll inflation along a plateau-like scalar potential within the framework of fluctuation-dissipation dynamics. We consider, in particular, that inflation was preceded by a radiation-dominated epoch where the inflaton is coupled to light degrees of freedom and may reach a near-equilibrium state. We show that the homogeneous field component can be sufficiently localized at the origin to trigger a period of slow-roll if the interactions between the inflaton and the thermal degrees of freedom are sufficiently strong and argue that this does not necessarily spoil the flatness of the potential at the quantum level. We further conclude that the inflaton can still be held at the origin after its potential begins to dominate the energy balance, leading to a period of thermal inflation. This then suppresses the effects of nonlinear interactions between the homogeneous and inhomogeneous field modes that could prevent the former from entering a slow-roll regime. Finally, we discuss the possibility of an early period of chaotic inflation, at large field values, followed by a first stage of reheating and subsequently by a second inflationary epoch along the plateau about the origin. This scenario could prevent an early overclosure of the Universe, at the same time yielding a low tensor-to-scalar ratio in agreement with observations.
Peer review: yes
URI: http://hdl.handle.net/10773/24029
DOI: 10.1088/1475-7516/2018/01/002
ISSN: 1475-7516
Appears in Collections:CIDMA - Artigos

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