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  • Access by Xinjiang University

Cosmic-ray cooling by dark matter in astrophysical jets

Dimitrios Kantzas1,2,*, Francesca Calore1,†, and Marco Chianese3,4,‡

  • 1LAPTh, CNRS, USMB, F-74940 Annecy, France
  • 2Center for Astrophysics and Space Science (CASS), New York University Abu Dhabi, PO Box 129188, Abu Dhabi, United Arab Emirates
  • 3Scuola Superiore Meridionale, Via Mezzocannone 4, I-80138 Napoli, Italy
  • 4INFN—Sezione di Napoli, Complesso Universitario Monte Sant’Angelo, I-80126 Napoli, Italy

  • *Contact author: dimitrios.kantzas@nyu.edu
  • Contact author: calore@lapth.cnrs.fr
  • Contact author: m.chianese@ssmeridionale.it

Phys. Rev. D 113, 023048 – Published 26 January, 2026

DOI: https://doi.org/10.1103/fbfw-ptcw

Abstract

Astrophysical jets from powerful active galactic nuclei (AGN) have recently been proposed as promising probes of dark matter (DM) in the sub-GeV mass range. AGN launch relativistic jets that accelerate cosmic rays (CRs) to very high energies, which can then interact with their surroundings and produce multiwavelength (MW) emission spanning from radio frequencies to TeV γ rays. If DM consists of light particles, their interactions with CRs could lead to an additional cooling mechanism that modifies the expected MW emission. In this work, we analyze the MW spectrum of Markarian 421, a well-studied AGN, using a multizone leptonic jet model that includes the interactions between CR electrons and DM particles. For the first time, we account for the uncertainties in the astrophysical jet dynamics, which have been previously neglected when constraining the CR-DM interactions. By fitting simultaneously jet parameters and DM-electrons interactions, we use the MW data from Markarian 421 to set constraints on the DM-induced CR cooling. We obtain 5σ upper limit σDMe1×1034cm2 for a DM mass of 1 MeV. We demonstrate that this is about a factor of 2–10 stronger than traditional approaches depending on DM mass. This improvement originates from having indeed considered the full multiwavelength emission from the source, instead if a simplified approach. Properly accounting for degeneracies between jet dynamics and DM interactions is also key to deriving robust constraints on DM interactions.

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