Implications of CoGeNT and DAMA for light WIMP dark matter
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Implications of CoGeNT’s new results for dark matterResults from a low-energy analysis of the CDMS II germanium data.Can neutralinos in the MSSM and NMSSM scenarios still be light?Light WIMPs in the Sun: Constraints from helioseismologyLight asymmetric dark matter from new strong dynamicsOn the potentiality of the ZnWO4 anisotropic detectors to measure the directionality of Dark MatterOn corollary model-dependent analyses and comparisonsDARK MATTER INVESTIGATION BY DAMA AT GRAN SASSONew Directions in Direct Dark Matter SearchesSearching for dark matter via mono- $$Z$$ Z boson production at the ILC
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Implications of CoGeNT and DAMA for light WIMP dark matter
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2010 nî lūn-bûn
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2010 թուականի Յունիսին հրատարակուած գիտական յօդուած
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2010 թվականի հունիսին հրատարակված գիտական հոդված
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2010年の論文
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2010年論文
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2010年論文
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2010年論文
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2010年論文
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2010年論文
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2010年论文
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name
Implications of CoGeNT and DAMA for light WIMP dark matter
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Implications of CoGeNT and DAMA for light WIMP dark matter
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Implications of CoGeNT and DAMA for light WIMP dark matter
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Implications of CoGeNT and DAMA for light WIMP dark matter
@ast
Implications of CoGeNT and DAMA for light WIMP dark matter
@en
Implications of CoGeNT and DAMA for light WIMP dark matter
@nl
prefLabel
Implications of CoGeNT and DAMA for light WIMP dark matter
@ast
Implications of CoGeNT and DAMA for light WIMP dark matter
@en
Implications of CoGeNT and DAMA for light WIMP dark matter
@nl
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Implications of CoGeNT and DAMA for light WIMP dark matter
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A. Liam Fitzpatrick
Dan Hooper
Kathryn M. Zurek
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10.1103/PHYSREVD.81.115005
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2010-06-11T00:00:00Z