Halo uncertainties in electron recoil events at direct detection experiments
Abstract The dark matter direct detection rates are highly correlated with the phase space distribution of dark matter particles in our galactic neighbourhood. In this paper we make a systematic study of the impact of astrophysical uncertainties on electron recoil events at the direct detection expe...
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2021
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oai:doaj.org-article:e69e0afbd65f4c56bdbd6110365f53802021-11-14T12:13:37ZHalo uncertainties in electron recoil events at direct detection experiments10.1140/epjc/s10052-021-09805-21434-60441434-6052https://doaj.org/article/e69e0afbd65f4c56bdbd6110365f53802021-11-01T00:00:00Zhttps://doi.org/10.1140/epjc/s10052-021-09805-2https://doaj.org/toc/1434-6044https://doaj.org/toc/1434-6052Abstract The dark matter direct detection rates are highly correlated with the phase space distribution of dark matter particles in our galactic neighbourhood. In this paper we make a systematic study of the impact of astrophysical uncertainties on electron recoil events at the direct detection experiments with Xenon and semiconductor detectors. We find that within the standard halo model there can be up to $$ \sim 50\%$$ ∼ 50 % deviation from the fiducial choice in the exclusion bounds from these observational uncertainties. For non-standard halo models we report a similar deviation from the fiducial standard halo model when fitted with recent cosmological N-body simulations while even larger deviations are obtained in case of the observational uncertainties.Tarak Nath MaityTirtha Sankar RaySambo SarkarSpringerOpenarticleAstrophysicsQB460-466Nuclear and particle physics. Atomic energy. RadioactivityQC770-798ENEuropean Physical Journal C: Particles and Fields, Vol 81, Iss 11, Pp 1-19 (2021) |
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Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
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Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Tarak Nath Maity Tirtha Sankar Ray Sambo Sarkar Halo uncertainties in electron recoil events at direct detection experiments |
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Abstract The dark matter direct detection rates are highly correlated with the phase space distribution of dark matter particles in our galactic neighbourhood. In this paper we make a systematic study of the impact of astrophysical uncertainties on electron recoil events at the direct detection experiments with Xenon and semiconductor detectors. We find that within the standard halo model there can be up to $$ \sim 50\%$$ ∼ 50 % deviation from the fiducial choice in the exclusion bounds from these observational uncertainties. For non-standard halo models we report a similar deviation from the fiducial standard halo model when fitted with recent cosmological N-body simulations while even larger deviations are obtained in case of the observational uncertainties. |
format |
article |
author |
Tarak Nath Maity Tirtha Sankar Ray Sambo Sarkar |
author_facet |
Tarak Nath Maity Tirtha Sankar Ray Sambo Sarkar |
author_sort |
Tarak Nath Maity |
title |
Halo uncertainties in electron recoil events at direct detection experiments |
title_short |
Halo uncertainties in electron recoil events at direct detection experiments |
title_full |
Halo uncertainties in electron recoil events at direct detection experiments |
title_fullStr |
Halo uncertainties in electron recoil events at direct detection experiments |
title_full_unstemmed |
Halo uncertainties in electron recoil events at direct detection experiments |
title_sort |
halo uncertainties in electron recoil events at direct detection experiments |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/e69e0afbd65f4c56bdbd6110365f5380 |
work_keys_str_mv |
AT taraknathmaity halouncertaintiesinelectronrecoileventsatdirectdetectionexperiments AT tirthasankarray halouncertaintiesinelectronrecoileventsatdirectdetectionexperiments AT sambosarkar halouncertaintiesinelectronrecoileventsatdirectdetectionexperiments |
_version_ |
1718429378584510464 |