Boosted dark matter quarrying at surface neutrino detectors
Abstract We propose the idea of “Earth Shielding” to reject cosmic-ray backgrounds, in the search for boosted dark matter at surface neutrino detectors, resulting in the enhancement of the signal-to-background ratio. The identification of cosmic-originating rare signals, especially lacking features,...
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Online Access: | http://link.springer.com/article/10.1007/JHEP08(2018)155 |
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doaj-65ae6f6b7c8d482f9135654570e1db3c2020-11-25T00:54:44ZengSpringerOpenJournal of High Energy Physics1029-84792018-08-012018812410.1007/JHEP08(2018)155Boosted dark matter quarrying at surface neutrino detectorsDoojin Kim0Kyoungchul Kong1Jong-Chul Park2Seodong Shin3Theoretical Physics Department, CERNDepartment of Physics and Astronomy, University of KansasDepartment of Physics, Chungnam National UniversityEnrico Fermi Institute, University of ChicagoAbstract We propose the idea of “Earth Shielding” to reject cosmic-ray backgrounds, in the search for boosted dark matter at surface neutrino detectors, resulting in the enhancement of the signal-to-background ratio. The identification of cosmic-originating rare signals, especially lacking features, at surface detectors is often considered hopeless due to a vast amount of cosmic-ray-induced background, hence underground experiments are better motivated to avoid such a challenge. We claim that surface detectors can attain remarkable sensitivities to even featureless signals, once restricting to events coming through the Earth from the opposite side of the detector location for the signals leaving appreciable tracks from which the source direction is inferred. By doing so, potential backgrounds in the signal region of interest can be substantially suppressed. To validate our claim, we study experimental reaches at several surface experiments such as SBN Program (MicroBooNE, ICARUS, and SBND) and ProtoDUNE for elastic boosted dark matter signatures stemming from the Galactic Center. We provide a systematic discussion on maximizing associated signal sensitivities.http://link.springer.com/article/10.1007/JHEP08(2018)155Beyond Standard ModelCosmology of Theories beyond the SM |
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DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Doojin Kim Kyoungchul Kong Jong-Chul Park Seodong Shin |
spellingShingle |
Doojin Kim Kyoungchul Kong Jong-Chul Park Seodong Shin Boosted dark matter quarrying at surface neutrino detectors Journal of High Energy Physics Beyond Standard Model Cosmology of Theories beyond the SM |
author_facet |
Doojin Kim Kyoungchul Kong Jong-Chul Park Seodong Shin |
author_sort |
Doojin Kim |
title |
Boosted dark matter quarrying at surface neutrino detectors |
title_short |
Boosted dark matter quarrying at surface neutrino detectors |
title_full |
Boosted dark matter quarrying at surface neutrino detectors |
title_fullStr |
Boosted dark matter quarrying at surface neutrino detectors |
title_full_unstemmed |
Boosted dark matter quarrying at surface neutrino detectors |
title_sort |
boosted dark matter quarrying at surface neutrino detectors |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2018-08-01 |
description |
Abstract We propose the idea of “Earth Shielding” to reject cosmic-ray backgrounds, in the search for boosted dark matter at surface neutrino detectors, resulting in the enhancement of the signal-to-background ratio. The identification of cosmic-originating rare signals, especially lacking features, at surface detectors is often considered hopeless due to a vast amount of cosmic-ray-induced background, hence underground experiments are better motivated to avoid such a challenge. We claim that surface detectors can attain remarkable sensitivities to even featureless signals, once restricting to events coming through the Earth from the opposite side of the detector location for the signals leaving appreciable tracks from which the source direction is inferred. By doing so, potential backgrounds in the signal region of interest can be substantially suppressed. To validate our claim, we study experimental reaches at several surface experiments such as SBN Program (MicroBooNE, ICARUS, and SBND) and ProtoDUNE for elastic boosted dark matter signatures stemming from the Galactic Center. We provide a systematic discussion on maximizing associated signal sensitivities. |
topic |
Beyond Standard Model Cosmology of Theories beyond the SM |
url |
http://link.springer.com/article/10.1007/JHEP08(2018)155 |
work_keys_str_mv |
AT doojinkim boosteddarkmatterquarryingatsurfaceneutrinodetectors AT kyoungchulkong boosteddarkmatterquarryingatsurfaceneutrinodetectors AT jongchulpark boosteddarkmatterquarryingatsurfaceneutrinodetectors AT seodongshin boosteddarkmatterquarryingatsurfaceneutrinodetectors |
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1725232907003363328 |