Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments

We reinterpret the results of the direct searches for dark matter in terms of milli-interacting dark particles. The model reproduces the positive results from DAMA/LIBRA and CoGeNT and is consistent with the absence of signal in the XENON100, CDMS-II/Ge, and LUX detectors. Dark atoms, interacting wi...

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Main Author: Quentin Wallemacq
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/525208
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author Quentin Wallemacq
author_facet Quentin Wallemacq
author_sort Quentin Wallemacq
collection DOAJ
description We reinterpret the results of the direct searches for dark matter in terms of milli-interacting dark particles. The model reproduces the positive results from DAMA/LIBRA and CoGeNT and is consistent with the absence of signal in the XENON100, CDMS-II/Ge, and LUX detectors. Dark atoms, interacting with standard atoms through a kinetic mixing between photons and dark photons and a mass mixing of σ mesons with dark scalars, diffuse elastically in terrestrial matter where they deposit all their energy. Reaching underground detectors through gravity at thermal energies, they form bound states with nuclei of the active medium by radiative capture, which causes the emission of photons that produce the observed signals. The parameter space of the model is explored and regions reproducing the results at the 2σ level are obtained for each experiment.
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spelling doaj-art-f7e55251618f4d6180f57268ba7799952025-02-03T07:23:32ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/525208525208Milli-Interacting Dark Matter Interpretation of the Direct-Search ExperimentsQuentin Wallemacq0IFPA, AGO Department, University of Liège, Sart Tilman, 4000 Liège, BelgiumWe reinterpret the results of the direct searches for dark matter in terms of milli-interacting dark particles. The model reproduces the positive results from DAMA/LIBRA and CoGeNT and is consistent with the absence of signal in the XENON100, CDMS-II/Ge, and LUX detectors. Dark atoms, interacting with standard atoms through a kinetic mixing between photons and dark photons and a mass mixing of σ mesons with dark scalars, diffuse elastically in terrestrial matter where they deposit all their energy. Reaching underground detectors through gravity at thermal energies, they form bound states with nuclei of the active medium by radiative capture, which causes the emission of photons that produce the observed signals. The parameter space of the model is explored and regions reproducing the results at the 2σ level are obtained for each experiment.http://dx.doi.org/10.1155/2014/525208
spellingShingle Quentin Wallemacq
Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments
Advances in High Energy Physics
title Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments
title_full Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments
title_fullStr Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments
title_full_unstemmed Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments
title_short Milli-Interacting Dark Matter Interpretation of the Direct-Search Experiments
title_sort milli interacting dark matter interpretation of the direct search experiments
url http://dx.doi.org/10.1155/2014/525208
work_keys_str_mv AT quentinwallemacq milliinteractingdarkmatterinterpretationofthedirectsearchexperiments