CosmiXs: Improved spectra for dark matter indirect detection
Chiara Arina, Mattia Di Mauro, Nicolao Fornengo, Jan Heisig, Adil, Jueid, Roberto Ruiz de Austri

TL;DR
This paper presents enhanced calculations of dark matter annihilation spectra incorporating electroweak effects, helicity information, and improved hadronization modeling, providing more accurate inputs for indirect detection analyses.
Contribution
It introduces a novel approach using helicity-dependent antenna showers and updated fragmentation tuning to improve spectral predictions for dark matter annihilation.
Findings
Inclusion of electroweak radiation effects in spectra calculations.
Implementation of helicity-dependent showering with Vincia.
Public release of spectra for dark matter masses 5-100 GeV.
Abstract
The spectra of stable particles produced from dark matter (DM) are one of the most important ingredients to calculate the fluxes for DM indirect detection experiments. At energies above a few GeV, most of the particles are produced following a complex sequence of phenomena including resonance decays, QED and QCD final-state radiation, radiation of weak gauge bosons, hadronization and hadron decays. In this contribution, we discuss improvements on the calculation of the energy spectra at the source using state-of-the-art tools that include effects that were not taken previously into account. We include helicity information of the particles produced in the annihilation channels, which leads to proper inclusion of electroweak radiation during the entire showering history. These effects are taken into account using the Vincia, which is based on the helicity-dependent antenna shower…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · CCD and CMOS Imaging Sensors · Astronomy and Astrophysical Research
