BBN Constraints on the Hadronic Annihilation of sub-GeV Dark Matter
arXiv:2510.11791 · doi:10.1103/b5wj-jw62
Abstract
We investigate the impact of residual annihilation from sub-GeV mass thermal relic dark matter candidates during big bang nucleosynthesis (BBN). Focusing on candidates with -wave annihilation channels, we show that the hadronic injection of pions and kaons beyond freeze-out, and their subsequent interaction with protons and neutrons prior to the deuterium bottleneck, provides a sensitivity to annihilation that surpasses that of the CMB and indirect detection in the galaxy.
arXiv comment7 pages, 5 figures. Minor corrections to Fig. 5
References in corpus (47)
- Big Bang Nucleosynthesis: 2015
- Scalar Dark Matter candidates
- One percent determination of the primordial deuterium abundance
- Big Bang nucleosynthesis and physics beyond the Standard Model
- CMB Constraints on WIMP Annihilation: Energy Absorption During the Recombination Epoch
- Primordial Nucleosynthesis: from precision cosmology to fundamental physics
- Big-Bang Nucleosynthesis and Gravitino
- Primordial Nucleosynthesis: Theory and Observations
- Big Bang Nucleosynthesis Constraints on Hadronically and Electromagnetically Decaying Relic Neutral Particles
- Big-Bang Nucleosynthesis and the Baryon Density of the Universe
- Big-Bang Nucleosynthesis After Planck
- Big-bang Nucleosynthesis Enters the Precision Era
- Results on light dark matter particles with a low-threshold CRESST-II detector
- Precision measures of the primordial abundance of deuterium
- Relic neutrino decoupling with flavour oscillations revisited
- Search for Invisible Decays of a Dark Photon Produced in e+e- Collisions at BaBar
- Primordial Lithium and Big Bang Nucleosynthesis
- Probing a Secluded U(1) at B-factories
- Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?
- Nuclear Reaction Network for Primordial Nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields
- Revisiting Big-Bang Nucleosynthesis Constraints on Long-Lived Decaying Particles
- Dark Matter, Millicharges, Axion and Scalar Particles, Gauge Bosons, and Other New Physics with LDMX
- Big Bang Nucleosynthesis as a Probe of New Physics
- Big Bang Nucleosynthesis and Particle Dark Matter
- Current Dark Matter Annihilation Constraints from CMB and Low-Redshift Data
- Refined Bounds on MeV-scale Thermal Dark Sectors from BBN and the CMB
- Neutrino decoupling beyond the Standard Model: CMB constraints on the Dark Matter mass with a fast and precise evaluation
- Signatures of sub-GeV dark matter beams at neutrino experiments
- BBN for the LHC: constraints on lifetimes of the Higgs portal scalars
- The PHLEK Survey: A New Determination of the Primordial Helium Abundance
- Improving Helium Abundance Determinations with Leo P as a Case Study
- BBN constraints on the annihilation of MeV-scale dark matter
- The primordial deuterium abundance: subDLA system at towards the QSO J1444+2919
- A robust deuterium abundance; Re-measurement of the z=3.256 absorption system towards the quasar PKS1937-1009
- Determination of the primordial helium abundance based on NGC 346 an HII region of the Small Magellanic Cloud
- Metastable GeV-scale particles as a solution to the cosmological lithium problem
- A precise deuterium abundance: Re-measurement of the z=3.572 absorption system towards the quasar PKS1937-101
- A new determination of the primordial helium abundance using the analyses of HII region spectra from SDSS
- A Bayesian direct method implementation to fit emission line spectra: Application to the primordial He abundance determination
- The primordial deuterium abundance at z = 2.504 from a high signal-to-noise spectrum of Q1009+2956
- Chemical abundances in 7 metal-poor HII regions and a determination of the primordial helium abundance
- Robust cosmic-ray constraints on -wave annihilating MeV dark matter
- Towards a full description of MeV dark matter decoupling: a self-consistent determination of relic abundance and
- Prospects for indirect MeV Dark Matter detection with Gamma Rays in light of Cosmic Microwave Background Constraints
- Extragalactic 85Rb/87Rb and 6Li/7Li ratios in the Small Magellanic Cloud
- Early Dark Energy During Big Bang Nucleosynthesis
- Revisiting big bang nucleosynthesis with a new particle species : effect of co-annihilation with nucleons