Initial conditions for the Galileon dark energy
Cristiano Germani (ICC, Universitat de Barcelona)

TL;DR
This paper investigates the initial conditions for Galileon dark energy models, revealing quantum effects can influence classical trajectories and constraining the universe's reheating temperature based on these models.
Contribution
It analyzes the impact of quantum effects on classical Galileon trajectories and establishes bounds on the reheating temperature from initial condition constraints.
Findings
Quantum effects can dominate classical trajectories in Galileon models.
Initial conditions on the tracker are ruled out during the radiation era.
Reheating temperature is constrained to be below 10^8 GeV.
Abstract
Galileon models are among the most appealing candidates for Dark Energy. The reason is twofold: classically, they provide a tracking solution leading to an almost DeSitter space starting from very generic initial conditions in the deep radiation era. The second reason is the standard lore that Galileons are quantum mechanically stable. The latter property is certainly true in flat space-time, thanks to the non-renormalization theorems of galilean coupling constants. However, in a cosmological background, we show that quantum effects might dominate the classical trajectory. Assuming the radiation era to last at least up to the electroweak phase transition, the trajectory with initial conditions sitting on the tracker is ruled out. On the other hand, it is always possible to find a sub-space of initial conditions such that the dark energy solution approaches stably the tracker at late…
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