Sommerfeld enhancement at NLO and the dark matter unitarity bound

We reexamine the consequences of perturbative unitarity on dark matter freeze-out when both Sommerfeld enhancement and bound state formation affect dark matter annihilations. At leading order the annihilation cross section is infrared dominated and the connection between the unitarity bound and the upper bound on the dark matter mass depends only on how the different partial waves are populated. We compute how this picture is modified at next-to-leading order with the goal of assigning a reliable theory uncertainty to the freeze-out predictions. We explicitly compute next-to-leading order corrections in a simple model with Abelian gauge interactions and provide an estimate of the theoretical uncertainty for the thermal masses of heavy electroweak <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>n</a:mi></a:math>-plets. Along the way, we clarify the regularization and matching procedure necessary to deal with singular potentials in quantum mechanics with a calculable, relativistic UV completion. Published by the American Physical Society 2024

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-10-28
DOI
https://doi.org/10.1103/physrevd.110.076027
Citations
5
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
3.30

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article

Sommerfeld enhancement at NLO and the dark matter unitarity bound

Diego Redigolo, Salvatore Bottaro
5 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
3.30
article

Sommerfeld enhancement at NLO and the dark matter unitarity bound

Diego Redigolo, Salvatore Bottaro
article en
5 citations

Abstract

We reexamine the consequences of perturbative unitarity on dark matter freeze-out when both Sommerfeld enhancement and bound state formation affect dark matter annihilations. At leading order the annihilation cross section is infrared dominated and the connection between the unitarity bound and the upper bound on the dark matter mass depends only on how the different partial waves are populated. We compute how this picture is modified at next-to-leading order with the goal of assigning a reliable theory uncertainty to the freeze-out predictions. We explicitly compute next-to-leading order corrections in a simple model with Abelian gauge interactions and provide an estimate of the theoretical uncertainty for the thermal masses of heavy electroweak <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>n</a:mi></a:math>-plets. Along the way, we clarify the regularization and matching procedure necessary to deal with singular potentials in quantum mechanics with a calculable, relativistic UV completion. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(7)
Tel Aviv University (IL), Istituto Nazionale di Fisica Nucleare, Sezione di Firenze (IT)
CERN, Israel Academy of Sciences and Humanities, Council for Higher Education
Openalex Percentile: Top 6%
Dark Matter and Cosmic Phenomena
3.30
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Sommerfeld enhancement at NLO and the dark matter unitarity bound — Diego Redigolo, Salvatore Bottaro · Physical review. D/Physical review. D. (2024) | TGRS Research Map | TGRS