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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Main Authors: Doojin Kim, Kyoungchul Kong, Jong-Chul Park, Seodong Shin
Format: Article
Language:English
Published: SpringerOpen 2018-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP08(2018)155
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spelling 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
collection 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
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AT kyoungchulkong boosteddarkmatterquarryingatsurfaceneutrinodetectors
AT jongchulpark boosteddarkmatterquarryingatsurfaceneutrinodetectors
AT seodongshin boosteddarkmatterquarryingatsurfaceneutrinodetectors
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