On the Occurrence of Finite-time Singularities in Swampland-related Quintessence Dark Energy Models
arXiv:2108.11324 · doi:10.1142/S0219887821502078
Abstract
In this work we focus on the phase space singularities of interactive quintessence model in the presence of matter fluid. This model is related to swampland studies, that the outcomes affect all these Swampland related models with the same dynamical system. We shall form the dynamical system corresponding to the cosmological system, which is eventually autonomous, and by using the dominant balances technique we shall investigate the occurrence or not of finite-time singularities. Our results indicate that the dynamical system of the model may develop finite-time singularities, but these are not general singularities, like in the case that the matter fluids were absent, in which case singularities occurred for general initial conditions. Hence, the presence of matter fluids affects the dynamical system of the cosmological system, making the singularities to depend on the initial conditions, instead of occurring for general initial conditions.
IJGMMP Accepted
References in corpus (12)
- On the Geometry of the String Landscape and the Swampland
- The Swampland: Introduction and Review
- The String Landscape and the Swampland
- Swampland Implications of GW170817-compatible Einstein-Gauss-Bonnet Gravity
- Rescaled Einstein-Hilbert Gravity from Gravity: Inflation, Dark Energy and the Swampland Criteria
- Dark energy beyond quintessence: Constraints from the swampland
- Higgs Inflation and the Refined dS Conjecture
- Reheating Constraints on Inflaton, Dark Matter: Swampland Conjecture
- The Swampland Conjectures and Slow-Roll Thawing Quintessence
- Rescaled Einstein-Hilbert Gravity: Inflation and the Swampland Criteria
- Revisiting Scalar Tensor inflation by swampland criteria and Reheating
- Implications of single field inflation in general cosmological scenarios on the nature of dark energy given the swampland conjectures