Abstract
We reexamine -essence dark energy models with a scalar field and a factorized Lagrangian, , with . A value of the equation of state parameter, , near requires either or . Previous work showed that thawing models with evolve along a set of unique trajectories for , while those with can result in a variety of different forms for . We show that if is small and is roughly constant, then the latter models also converge toward a single unique set of behaviors for , different from those with . We derive the functional form for in this case, determine the conditions on for which it applies, and present observational constraints on this new class of models. We note that -essence models with correspond to a dark energy sound speed .
- Received 15 May 2019
DOI:https://doi.org/10.1103/PhysRevD.100.023525
© 2019 American Physical Society