Quintom Cosmology: Theoretical implications and observations
Yi-Fu Cai, Emmanuel N. Saridakis, Mohammad R. Setare, and Jun-Qing Xia

TL;DR
This paper reviews quintom cosmology, exploring its theoretical foundations, observational implications, and various models, including scalar fields, higher derivative systems, and braneworld scenarios, highlighting its potential to explain dark energy dynamics.
Contribution
It provides a comprehensive review of quintom models, including a no-go theorem, alternative realizations, and implications for universe evolution, advancing understanding of dark energy crossing the cosmological constant boundary.
Findings
Double-field quintom models can fit current observations.
Higher derivative and non-scalar systems offer viable quintom realizations.
Quintom scenarios can lead to bouncing or oscillating universes.
Abstract
We review the paradigm of quintom cosmology. This scenario is motivated by the observational indications that the equation of state of dark energy across the cosmological constant boundary is mildly favored, although the data are still far from being conclusive. As a theoretical setup we introduce a no-go theorem existing in quintom cosmology, and based on it we discuss the conditions for the equation of state of dark energy realizing the quintom scenario. The simplest quintom model can be achieved by introducing two scalar fields with one being quintessence and the other phantom. Based on the double-field quintom model we perform a detailed analysis of dark energy perturbations and we discuss their effects on current observations. This type of scenarios usually suffer from a manifest problem due to the existence of a ghost degree of freedom, and thus we review various alternative…
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