Peer-reviewedCC BYJournal of Cosmology and Astroparticle Physics
Indirect searches for dark photon-photon tridents in celestial objects
- 1Stockholm University and The Oskar Klein Centre for Cosmoparticle Physics, Alba Nova, 10691 Stockholm,
- 2Institute of Physics, Academia Sinica, Nangang, Taipei 11529,
- 3Department of Physics and Astronomy, University of California, Irvine, CA 92697-4575,
Abstract
We model and constrain the unique indirect detection signature produced by dark matter particles that annihilate through a U(1) gauge symmetry into dark photons that subsequently decay into three-photon final states. We focus on scenarios where the dark photon is long-lived, and show that γ-ray probes of celestial objects can set strong constraints on the dark matter/baryon scattering cross section that in many cases surpass the power of current direct detection constraints, and in some cases even peer into the neutrino fog.
Related
- Searching for dark photon tridents through primordial black hole signatures
- Low-energy antinuclei measurements for background-free indirect dark matter searches and PBH signatures
- Direct and Indirect searches for DM-electron interactions in sub-GeV DM models
- Invisible dark-sector radiation: analytic resummation for dark photon searches
- Production Shape Effects Beyond Rate Rescaling in Dark Photon Searches
BibTeX
@article{linden2026indirect,
title = {{Indirect searches for dark photon-photon tridents in celestial objects}},
author = {Tim Linden and Thong T. Q. Nguyen and Tim M. P. Tait},
journal = {Journal of Cosmology and Astroparticle Physics},
year = {2026},
month = aug,
doi = {10.1088/1475-7516/2026/08/056},
url = {https://doi.org/10.1088/1475-7516/2026/08/056},
note = {CC BY},
}
RIS
TY - JOUR
TI - Indirect searches for dark photon-photon tridents in celestial objects
AU - Tim Linden
AU - Thong T. Q. Nguyen
AU - Tim M. P. Tait
PY - 2026
DA - 2026/08/01
JO - Journal of Cosmology and Astroparticle Physics
DO - 10.1088/1475-7516/2026/08/056
UR - https://doi.org/10.1088/1475-7516/2026/08/056
AB - We model and constrain the unique indirect detection signature produced by dark matter particles that annihilate through a U(1) gauge symmetry into dark photons that subsequently decay into three-photon final states. We focus on scenarios where the dark photon is long-lived, and show that γ-ray probes of celestial objects can set strong constraints on the dark matter/baryon scattering cross section that in many cases surpass the power of current direct detection constraints, and in some cases even peer into the neutrino fog.
SN - 1475-7508
SN - 1475-7516
ER -