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Unified phantom cosmology: inflation, dark energy and dark matter under the same standard
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Unified phantom cosmology: inflation, dark energy and dark matter under the same standard
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Phantom cosmology allows to account for dynamics and matter content of the universe tracing back the evolution to the inflationary epoch, considering the transition to the non-phantom standard cosmology (radiation/matter dominated eras) and recovering the today observed dark energy epoch. We develop the unified phantom cosmology where the same scalar plays the role of early time (phantom) inflaton and late-time Dark Energy. The recent transition from decelerating to accelerating phase is described too by the same scalar field. The (dark) matter may be embedded in this scheme, giving the natural solution of the coincidence problem. It is explained how the proposed unified phantom cosmology can be fitted against the observations which opens the way to define all the important parameters of the model.
Forward citations
Cited by 3 Pith papers
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ACT-DR6 consistent inflation in generalised entropic cosmology and $f(Q)$ gravity
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Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models
Phantom-to-quintessence crossing is impossible for a canonical scalar field, but can be engineered in finely-tuned k-essence theories where ghost instabilities are suppressed by a chosen kinetic coefficient.
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Modified gravity theories supply viable mathematical frameworks for inflation, bounces, and dark energy eras that match observational data.
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