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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Online Access: | http://link.springer.com/article/10.1007/JHEP08(2019)103 |
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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 |
work_keys_str_mv |
AT mbeneke resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution AT abroggio resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution AT chasner resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution AT kurban resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution AT mvollmann resummedphotonspectrumfromdarkmatterannihilationforintermediateandnarrowenergyresolution |
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1724509131624153088 |