Shielding of a direct detection experiment and implications for the DAMA annual modulation signal
Previous work has argued that, in the framework of plasma dark matter models, the DAMA annual modulation signal can be consistently explained with electron recoils. In the specific case of mirror dark matter, that explanation requires an effective low velocity cutoff, vc≳30,000km/s, for the halo mir...
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doaj-2b24b6a5dc104653a16feb752461472d2020-11-25T02:11:56ZengElsevierPhysics Letters B0370-26932019-02-01789592597Shielding of a direct detection experiment and implications for the DAMA annual modulation signalR. Foot0ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Sydney, NSW 2006, Australia; ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Melbourne, VIC 3010, Australia; Correspondence to: ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Melbourne, VIC 3010, Australia.Previous work has argued that, in the framework of plasma dark matter models, the DAMA annual modulation signal can be consistently explained with electron recoils. In the specific case of mirror dark matter, that explanation requires an effective low velocity cutoff, vc≳30,000km/s, for the halo mirror electron distribution at the detector. We show here that this cutoff can result from collisional shielding of the detector from the halo wind due to Earth-bound dark matter. We also show that shielding effects can reconcile the kinetic mixing parameter value inferred from direct detection experiments with the value favoured from small scale structure considerations, ϵ≈2×10−10.http://www.sciencedirect.com/science/article/pii/S0370269318310074 |
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DOAJ |
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English |
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Article |
sources |
DOAJ |
author |
R. Foot |
spellingShingle |
R. Foot Shielding of a direct detection experiment and implications for the DAMA annual modulation signal Physics Letters B |
author_facet |
R. Foot |
author_sort |
R. Foot |
title |
Shielding of a direct detection experiment and implications for the DAMA annual modulation signal |
title_short |
Shielding of a direct detection experiment and implications for the DAMA annual modulation signal |
title_full |
Shielding of a direct detection experiment and implications for the DAMA annual modulation signal |
title_fullStr |
Shielding of a direct detection experiment and implications for the DAMA annual modulation signal |
title_full_unstemmed |
Shielding of a direct detection experiment and implications for the DAMA annual modulation signal |
title_sort |
shielding of a direct detection experiment and implications for the dama annual modulation signal |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2019-02-01 |
description |
Previous work has argued that, in the framework of plasma dark matter models, the DAMA annual modulation signal can be consistently explained with electron recoils. In the specific case of mirror dark matter, that explanation requires an effective low velocity cutoff, vc≳30,000km/s, for the halo mirror electron distribution at the detector. We show here that this cutoff can result from collisional shielding of the detector from the halo wind due to Earth-bound dark matter. We also show that shielding effects can reconcile the kinetic mixing parameter value inferred from direct detection experiments with the value favoured from small scale structure considerations, ϵ≈2×10−10. |
url |
http://www.sciencedirect.com/science/article/pii/S0370269318310074 |
work_keys_str_mv |
AT rfoot shieldingofadirectdetectionexperimentandimplicationsforthedamaannualmodulationsignal |
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1724911768107483136 |