Resummed photon spectra for WIMP annihilation

Baumgart, Matthew; Cohen, Timothy; Moult, Ian; Rodd, Nicholas L.; Slatyer, Tracy R.; Solon, Mikhail P.; Stewart, Iain W.; Vaidya, Varun

doi:10.1007/JHEP03(2018)117

Title: Resummed photon spectra for WIMP annihilation

Journal Article · Tue Mar 20 04:00:00 UTC 2018 · Journal of High Energy Physics (Online)

DOI: https://doi.org/10.1007/JHEP03(2018)117 · OSTI ID:1440487

Baumgart, Matthew ^[1]; Cohen, Timothy ^[2]; Moult, Ian ^[3];

^[4];

^[4]; Solon, Mikhail P. ^[5]; Stewart, Iain W. ^[4]; Vaidya, Varun ^[6]

Arizona State Univ., Tempe, AZ (United States); Rutgers Univ., Piscataway, NJ (United States). New High Energy Theory Center
Univ. of Oregon, Eugene, OR (United States)
Univ. of California, Berkeley, CA (United States). Berkeley Center for Theoretical Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Theoretical Physics Group
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Center for Theoretical Physics
California Inst. of Technology (CalTech), Pasadena, CA (United States). Walter Burke Inst. for Theoretical Physics
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

We construct an effective field theory (EFT) description of the hard photon spectrum for heavy WIMP annihilation. This facilitates precision predictions relevant for line searches, and allows the incorporation of non-trivial energy resolution effects. Our framework combines techniques from non-relativistic EFTs and soft-collinear effective theory (SCET), as well as its multi-scale extensions that have been recently introduced for studying jet substructure. We find a number of interesting features, including the simultaneous presence of SCET_I and SCET_II modes, as well as collinear-soft modes at the electroweak scale. We derive a factorization formula that enables both the resummation of the leading large Sudakov double logarithms that appear in the perturbative spectrum, and the inclusion of Sommerfeld enhancement effects. Consistency of this factorization is demonstrated to leading logarithmic order through explicit calculation. Our final result contains both the exclusive and the inclusive limits, thereby providing a unifying description of these two previously-considered approximations. We estimate the impact on experimental sensitivity, focusing for concreteness on an SU(2) W triplet fermion dark matter — the pure wino — where the strongest constraints are due to a search for gamma-ray lines from the Galactic Center. Here, we find numerically significant corrections compared to previous results, thereby highlighting the importance of accounting for the photon spectrum when interpreting data from current and future indirect detection experiments.

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Research Organization:: Los Alamos National Lab. (LANL), Los Alamos, NM (United States); California Inst. of Technology (CalTech), Pasadena, CA (United States); Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: USDOE Laboratory Directed Research and Development (LDRD) Program; USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25); USDOE Office of Science (SC), Nuclear Physics (NP) (SC-26)

Grant/Contract Number:: AC52-06NA25396; AC02-05CH11231; SC0011632; SC0013999; SC0011090; SC0012567

OSTI ID:: 1440487

Report Number(s):: LA-UR--17-31169; CALT-TH--2017-066; MIT--CTP4959

Journal Information:: Journal of High Energy Physics (Online), Journal Name: Journal of High Energy Physics (Online) Journal Issue: 3 Vol. 2018; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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Search for γ -Ray Line Signals from Dark Matter Annihilations in the Inner Galactic Halo from 10 Years of Observations with H.E.S.S. Abdallah, H.; Abramowski, A.; Aharonian, F. Deutsches Elektronen-Synchrotron, DESY, Hamburg https://doi.org/10.3204/pubdb-2018-02055	text	January 2018
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