Quantum Quintom Cosmology
arXiv:2504.01741 · doi:10.1088/1475-7516/2025/07/048
Abstract
This work applies the principles of quantum cosmology to examine models incorporating a quintom field. Specifically, three distinct models are analyzed: a simplified toy model, a model featuring an exponential quintom potential, and one where the quintom field is coupled with a negative cosmological constant. For each case, we study the classical trajectories within the configuration space, present solutions to the Wheeler-DeWitt equation in quantum cosmology, and discuss physical interpretations and consequences. A key focus is the behavior of wave packets in the minisuperspace framework. Notably, the correspondence principle (connection between classical and quantum solutions) is also demonstrated. Furthermore, the appropriate quintom duality is introduced, and we discuss its consequences. A section including interesting and challenging discussions is also presented.
References in corpus (16)
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Quantum Nature of the Big Bang
- Can dark energy evolve to the Phantom?
- The Anthropic Landscape of String Theory
- Avoiding Dark Energy with 1/R Modifications of Gravity
- Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields
- Quantum phantom cosmology
- Quintom cosmologies admitting either tracking or phantom attractors
- Using the Noether symmetry approach to probe the nature of dark energy
- Quintom cosmology and modified gravity after DESI 2024
- Brane-world cosmology with black strings
- Phantom without UV pathology
- The Wheeler-DeWitt Quantization Can Solve the Singularity Problem
- Equivalence of cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection
- Wheeler-DeWitt equation and the applicability of crypto-Hermitian interaction representation in quantum cosmology
- A Wheeler-DeWitt Equation with Time