Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution

Abstract The annihilation cross section of weakly interacting TeV scale dark matter particles χ 0 into photons is affected by large quantum corrections due to electroweak Sudakov logarithms and the Sommerfeld effect. We extend our previous work on the resummation of the semi-inclusive photon energy...

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Main Authors: M. Beneke, A. Broggio, C. Hasner, K. Urban, M. Vollmann
Format: Article
Language:English
Published: SpringerOpen 2019-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP08(2019)103
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spelling doaj-04d8f81526594d84b0295ce355cf761d2020-11-25T03:45:53ZengSpringerOpenJournal of High Energy Physics1029-84792019-08-012019818610.1007/JHEP08(2019)103Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolutionM. Beneke0A. Broggio1C. Hasner2K. Urban3M. Vollmann4Physik Department T31, Technische Universität MünchenUniversità degli Studi di Milano-BicoccaPhysik Department T31, Technische Universität MünchenPhysik Department T31, Technische Universität MünchenPhysik Department T31, Technische Universität MünchenAbstract The annihilation cross section of weakly interacting TeV scale dark matter particles χ 0 into photons is affected by large quantum corrections due to electroweak Sudakov logarithms and the Sommerfeld effect. We extend our previous work on the resummation of the semi-inclusive photon energy spectrum in χ 0 χ 0 → γ + X in the vicinity of the maximal photon energy E γ = m χ with NLL’ accuracy from the case of narrow photon energy resolution E res γ $$ {E}_{\mathrm{res}}^{\gamma } $$ of order m W 2 / m χ $$ {m}_W^2/{m}_{\chi } $$ to intermediate resolution of order E res γ ∼ m W $$ {E}_{\mathrm{res}}^{\gamma}\sim {m}_W $$ . We also provide details on the previous narrow resolution calculation. The two calculations, performed in different effective field theory set-ups for the wino dark matter model, are then shown to match well, providing an accurate representation up to energy resolutions of about 300 GeV.http://link.springer.com/article/10.1007/JHEP08(2019)103NLO Computations
collection DOAJ
language English
format Article
sources DOAJ
author M. Beneke
A. Broggio
C. Hasner
K. Urban
M. Vollmann
spellingShingle M. Beneke
A. Broggio
C. Hasner
K. Urban
M. Vollmann
Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
Journal of High Energy Physics
NLO Computations
author_facet M. Beneke
A. Broggio
C. Hasner
K. Urban
M. Vollmann
author_sort M. Beneke
title Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
title_short Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
title_full Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
title_fullStr Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
title_full_unstemmed Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
title_sort resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2019-08-01
description Abstract The annihilation cross section of weakly interacting TeV scale dark matter particles χ 0 into photons is affected by large quantum corrections due to electroweak Sudakov logarithms and the Sommerfeld effect. We extend our previous work on the resummation of the semi-inclusive photon energy spectrum in χ 0 χ 0 → γ + X in the vicinity of the maximal photon energy E γ = m χ with NLL’ accuracy from the case of narrow photon energy resolution E res γ $$ {E}_{\mathrm{res}}^{\gamma } $$ of order m W 2 / m χ $$ {m}_W^2/{m}_{\chi } $$ to intermediate resolution of order E res γ ∼ m W $$ {E}_{\mathrm{res}}^{\gamma}\sim {m}_W $$ . We also provide details on the previous narrow resolution calculation. The two calculations, performed in different effective field theory set-ups for the wino dark matter model, are then shown to match well, providing an accurate representation up to energy resolutions of about 300 GeV.
topic NLO Computations
url http://link.springer.com/article/10.1007/JHEP08(2019)103
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AT kurban resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution
AT mvollmann resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution
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