The Strong Force meets the Dark Sector: a robust estimate of QCD uncertainties for anti-matter dark matter searches
Adil Jueid, Jochem Kip, Roberto Ruiz de Austri, Peter Skands

TL;DR
This paper quantifies QCD uncertainties in antimatter spectra from dark-matter annihilation, significantly impacting the interpretation of indirect detection signals and providing tools for more accurate dark-matter parameter estimation.
Contribution
It presents a comprehensive analysis of QCD uncertainties using Pythia 8 variations, offering a conservative estimate and practical tools for dark-matter indirect detection studies.
Findings
QCD uncertainties can cause up to 40 GeV variation in dark-matter mass estimates.
Uncertainties can lead to about 10% variation in annihilation cross section.
Provided tabulated spectra and code for incorporating QCD uncertainties in dark-matter analyses.
Abstract
In dark-matter annihilation channels to hadronic final states, stable particles -- such as positrons, photons, antiprotons, and antineutrinos -- are produced via complex sequences of phenomena including QED/QCD radiation, hadronisation, and hadron decays. These processes are normally modelled by Monte Carlo event generators whose limited accuracy imply intrinsic QCD uncertainties on the predictions for indirect-detection experiments like Fermi-LAT, Pamela, IceCube or AMS-02. In this article, we perform a complete analysis of QCD uncertainties in antimatter spectra from dark-matter annihilation, based on parametric variations of the Pythia 8 event generator. After performing several retunings of light-quark fragmentation functions, we define a set of variations that span a conservative estimate of the QCD uncertainties. We estimate the effects on antimatter spectra for various…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Scientific Computing and Data Management
