Precision Photon Spectra for Wino Annihilation
Matthew Baumgart, Timothy Cohen, Emmanuel Moulin, Ian Moult, Lucia, Rinchiuso, Nicholas L. Rodd, Tracy R. Slatyer, Iain W. Stewart, and Varun, Vaidya

TL;DR
This paper presents precise, next-to-leading logarithmic predictions for the hard photon spectrum from wino dark matter annihilation, crucial for interpreting indirect detection experiment data.
Contribution
It introduces a state-of-the-art calculation framework that combines resummation of large logarithms and Sommerfeld effects at NLL accuracy for wino annihilation spectra.
Findings
Resummation at NLL shows good convergence with 5% uncertainty.
Full spectrum analysis is more accurate than single endpoint approximation.
The method is adaptable to other dark matter models.
Abstract
We provide precise predictions for the hard photon spectrum resulting from neutral SU triplet (wino) dark matter annihilation. Our calculation is performed utilizing an effective field theory expansion around the endpoint region where the photon energy is near the wino mass. This has direct relevance to line searches at indirect detection experiments. We compute the spectrum at next-to-leading logarithmic (NLL) accuracy within the framework established by a factorization formula derived previously by our collaboration. This allows simultaneous resummation of large Sudakov logarithms (arising from a restricted final state) and Sommerfeld effects. Resummation at NLL accuracy shows good convergence of the perturbative series due to the smallness of the electroweak coupling constant - scale variation yields uncertainties on our NLL prediction at the level of . We highlight a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
