Precision photon spectra for wino annihilation

Baumgart, Matthew; Cohen, Timothy; Moulin, Emmanuel; Moult, Ian; Rinchiuso, Lucia; Rodd, Nicholas L.; Slatyer, Tracy R.; Stewart, Iain W.; Vaidya, Varun

doi:10.1007/JHEP01(2019)036

Title: Precision photon spectra for wino annihilation

Journal Article · Fri Jan 04 00:00:00 EST 2019 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/JHEP01(2019)036· OSTI ID:1530788

Baumgart, Matthew ^[1]; Cohen, Timothy ^[2]; Moulin, Emmanuel ^[3]; Moult, Ian ^[4]; Rinchiuso, Lucia ^[3];

^[5];

^[6]; Stewart, Iain W. ^[6]; Vaidya, Varun ^[7]

Arizona State Univ., Tempe, AZ (United States)
Univ. of Oregon, Eugene, OR (United States)
Université Paris-Saclay, Gif-sur-Yvette (France)
Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

We provide precise predictions for the hard photon spectrum resulting from neutral SU(2)W 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 5%. We highlight a number of interesting field theory effects that appear at NLL associated with the presence of electroweak symmetry breaking, which should have more general applicability. We also study the importance of using the full spectrum as compared with a single endpoint bin approximation when computing experimental limits. Our calculation provides a state of the art prediction for the hard photon spectrum that can be easily generalized to other DM candidates, allowing for the robust interpretation of data collected by current and future indirect detection experiments.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States); Univ. of Oregon, Eugene, OR (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Nuclear Physics (NP); USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Laboratory Directed Research and Development (LDRD) Program

Grant/Contract Number:: 89233218CNA000001; SC0000232627; SC0018191; SC0011640; AC02-05CH11231; SC00012567; SC0013999; SCD011090; AC52-06NA25396; SC0012567; SC0011090

OSTI ID:: 1530788

Alternate ID(s):: OSTI ID: 1596614

Report Number(s):: LA-UR-18-25972; MIT-CTP-5025

Journal Information:: Journal of High Energy Physics (Online), Vol. 2019, Issue 1; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

Citation Metrics:

Cited by: 25 works

Citation information provided by
Web of Science

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Testing dark matter with Cherenkov light — prospects of H.E.S.S. and CTA for exploring minimal supersymmetry Hryczuk, Andrzej; Jodłowski, Krzysztof; Moulin, Emmanuel Journal of High Energy Physics, Vol. 2019, Issue 10 https://doi.org/10.1007/jhep10(2019)043	journal	October 2019
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72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
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Title: Precision photon spectra for wino annihilation

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