A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions

We present Ph-[Formula: see text]CDM, a phantom-scalar realization within General Relativity of the sign-switching cosmological-constant idea, [Formula: see text]CDM, in which a phantom scalar evolving on a bounded hyperbolic-tangent potential induces a smooth mirror AdS-to-dS transition in the late-time dark-energy density. The wrong-sign kinetic term, usually viewed as pathological, becomes the mechanism lifting the field from a negative- to a positive-energy vacuum-like regime. The construction also shows that the field can become repulsive while its energy density is still negative. The cosmology nevertheless remains controlled: total energy stays positive, the late-time attractor is de Sitter rather than a Big Rip, and the dynamics remain safely infrared. Ph-[Formula: see text]CDM thus offers a concrete late-time mechanism with the potential to address multiple cosmological tensions.

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Publication Details

Journal
International Journal of Modern Physics D
Published
2026-08-25
DOI
https://doi.org/10.1142/s021827182641021x
Primary Topic
Cosmology and Gravitation Theories
Type
article
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article

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions

A. Emrah Yükselci, Alexander Zhuk, Leandros Perivolaropoulos, Özgür Akarsu
International Journal of Modern Physics D
Cosmology and Gravitation Theories
article

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions

A. Emrah Yükselci, Alexander Zhuk, Leandros Perivolaropoulos, Özgür Akarsu
article en

Abstract

We present Ph-[Formula: see text]CDM, a phantom-scalar realization within General Relativity of the sign-switching cosmological-constant idea, [Formula: see text]CDM, in which a phantom scalar evolving on a bounded hyperbolic-tangent potential induces a smooth mirror AdS-to-dS transition in the late-time dark-energy density. The wrong-sign kinetic term, usually viewed as pathological, becomes the mechanism lifting the field from a negative- to a positive-energy vacuum-like regime. The construction also shows that the field can become repulsive while its energy density is still negative. The cosmology nevertheless remains controlled: total energy stays positive, the late-time attractor is de Sitter rather than a Big Rip, and the dynamics remain safely infrared. Ph-[Formula: see text]CDM thus offers a concrete late-time mechanism with the potential to address multiple cosmological tensions.

International Journal of Modern Physics D
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