Kination and the Inert Doublet Model

Fuente: arXiv
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Main Authors: Bélanger, Geneviève, Bernal, Nicolás, Goudelis, Andreas, Pukhov, Alexander
Format: Preprint
Published: 2025
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author Bélanger, Geneviève
Bernal, Nicolás
Goudelis, Andreas
Pukhov, Alexander
author_facet Bélanger, Geneviève
Bernal, Nicolás
Goudelis, Andreas
Pukhov, Alexander
contents The inert doublet model is a two-Higgs-doublet extension of the standard model that provides a minimal and versatile framework for frozen-out dark matter. Assuming standard cosmology, if the dark matter mass ranges between approximately 120 GeV and 500 GeV then it turns out to be underabundant, as gauge interactions render its annihilation too efficient. In this work, we show that this mass window becomes allowed in cosmological scenarios where dark matter freeze-out occurs during a period with a stiff equation of state, $w > 1/3$, such as kination. This predictive setup satisfies all current experimental constraints while remaining within the reach of upcoming detection efforts.
format Preprint
id arxiv_https___arxiv_org_abs_2512_15864
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Kination and the Inert Doublet Model
Bélanger, Geneviève
Bernal, Nicolás
Goudelis, Andreas
Pukhov, Alexander
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
The inert doublet model is a two-Higgs-doublet extension of the standard model that provides a minimal and versatile framework for frozen-out dark matter. Assuming standard cosmology, if the dark matter mass ranges between approximately 120 GeV and 500 GeV then it turns out to be underabundant, as gauge interactions render its annihilation too efficient. In this work, we show that this mass window becomes allowed in cosmological scenarios where dark matter freeze-out occurs during a period with a stiff equation of state, $w > 1/3$, such as kination. This predictive setup satisfies all current experimental constraints while remaining within the reach of upcoming detection efforts.
title Kination and the Inert Doublet Model
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2512.15864