Connecting t-channel dark matter models to the Standard Model Effective Field Theory

A bstract We investigate the connection between simplified dark matter models featuring a t -channel scalar mediator and the Standard Model Effective Field Theory (SMEFT). We focus on scenarios with fermionic dark matter interacting with leptons, under the assumption of Minimal Flavor Violation. The dimension-six SMEFT Wilson coefficients are computed in the Warsaw basis at one loop, with the aid of Matchete. Assuming a compressed mass spectrum for the dark matter and the mediator, we incorporate coannihilations, Sommerfeld enhancement, and bound-state effects in the relic density calculation. We then analyze the interplay between the dark matter energy density, global SMEFT fits, and direct detection constraints. Our results show that SMEFT bounds, though loop-suppressed, can meaningfully constrain the parameter space for m χ ≳ 200 GeV and $$ \mathcal{O}(1) $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>O</mml:mi> <mml:mfenced> <mml:mn>1</mml:mn> </mml:mfenced> </mml:math> portal couplings.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-10-08
DOI
https://doi.org/10.1007/jhep10(2025)060
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

Connecting t-channel dark matter models to the Standard Model Effective Field Theory

O. Panella, Simone Biondini, Lorenzo Tiberi
Journal of High Energy Physics
Dark Matter and Cosmic Phenomena
article

Connecting t-channel dark matter models to the Standard Model Effective Field Theory

O. Panella, Simone Biondini, Lorenzo Tiberi
article en

Abstract

A bstract We investigate the connection between simplified dark matter models featuring a t -channel scalar mediator and the Standard Model Effective Field Theory (SMEFT). We focus on scenarios with fermionic dark matter interacting with leptons, under the assumption of Minimal Flavor Violation. The dimension-six SMEFT Wilson coefficients are computed in the Warsaw basis at one loop, with the aid of Matchete. Assuming a compressed mass spectrum for the dark matter and the mediator, we incorporate coannihilations, Sommerfeld enhancement, and bound-state effects in the relic density calculation. We then analyze the interplay between the dark matter energy density, global SMEFT fits, and direct detection constraints. Our results show that SMEFT bounds, though loop-suppressed, can meaningfully constrain the parameter space for m χ ≳ 200 GeV and $$ \mathcal{O}(1) $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>O</mml:mi> <mml:mfenced> <mml:mn>1</mml:mn> </mml:mfenced> </mml:math> portal couplings.

Journal of High Energy PhysicsVol. 2025(10)
University of Freiburg (DE), University of Perugia (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (IT)
Openalex Percentile: Top 87%
Dark Matter and Cosmic Phenomena
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