The simplest dark matter model at the edge of perturbativity

Increasingly sensitive direct detection dark matter experiments are testing important regions of parameter space for WIMP dark matter and pushing many models to the multi-TeV regime. This brings into question the perturbativity of these models. In this context, and in light of the new limits from the LZ experiment, we investigate the status of the simplest thermal dark matter model: a singlet scalar, real or complex, coupled to the Higgs boson. We calculate the next-to-leading order (NLO) corrections to the direct detection rates as well as for the annihilations driving thermal freeze-out. For the complex case, we find that the entire perturbative region is excluded by direct detection. For the real case we find that the mass should be ≳ 20 TeV at NLO, compared with the ≳ 30 TeV LO limit. We highlight that a three-fold improvement on WIMP spin independent interactions can fully test the real scalar model in the perturbative regime. Finally, for both models, there is still an allowed (albeit narrow) region near the Higgs resonance where couplings are perturbative.

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Publication Details

Journal
Physics Letters B
Published
2025-06-27
DOI
https://doi.org/10.1016/j.physletb.2025.139696
Citations
4
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
4.62
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article

The simplest dark matter model at the edge of perturbativity

Miguel Escudero, Thomas Hambye
4 citations
Physics Letters B
Cosmology and Gravitation Theories
4.62
article

The simplest dark matter model at the edge of perturbativity

Miguel Escudero, Thomas Hambye
article en
4 citations

Abstract

Increasingly sensitive direct detection dark matter experiments are testing important regions of parameter space for WIMP dark matter and pushing many models to the multi-TeV regime. This brings into question the perturbativity of these models. In this context, and in light of the new limits from the LZ experiment, we investigate the status of the simplest thermal dark matter model: a singlet scalar, real or complex, coupled to the Higgs boson. We calculate the next-to-leading order (NLO) corrections to the direct detection rates as well as for the annihilations driving thermal freeze-out. For the complex case, we find that the entire perturbative region is excluded by direct detection. For the real case we find that the mass should be ≳ 20 TeV at NLO, compared with the ≳ 30 TeV LO limit. We highlight that a three-fold improvement on WIMP spin independent interactions can fully test the real scalar model in the perturbative regime. Finally, for both models, there is still an allowed (albeit narrow) region near the Higgs resonance where couplings are perturbative.

Physics Letters BVol. 868
Université Libre de Bruxelles (BE), European Organization for Nuclear Research (CH)
Climate action
Openalex Percentile: Top 6%
Cosmology and Gravitation Theories
4.62
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The simplest dark matter model at the edge of perturbativity — Miguel Escudero, Thomas Hambye · Physics Letters B (2025) | TGRS Research Map | TGRS