2014
DOI: 10.1016/j.nima.2013.10.079
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DAMA/LIBRA results and perspectives of phase 2

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Cited by 16 publications
(9 citation statements)
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“…In Figure 6, the approximate sensitivities to m χ = 5 GeV/c 2 DM are plotted as vertical lines to illustrate the potential cumulative effect the dark disk, density wake, and kinematic wake can have for various experiments (see [4,7,[73][74][75] for sensitivity determinations, where E R has been translated to v min as in Section III B). Each experiment has been able to place limits on σ χ and m χ , with the earlier generation CDMS-Si experiment [74] finding three possible events that make the most likely model for a DM particle m χ = 8.6 GeV/c 2 and σ χ = 1.9 × 10 −41 cm 2 , consistent with the CoGeNT results [4], as well as the DAMA (Na) results [5]. We also plot horizontal lines connecting the vertical line at m χ = 5 GeV (right extent) to a limit at m χ = 10 GeV (left extent) as a function of v min to demonstrate the different values of dR/dv min each experiment would reasonably expect to observe.…”
Section: B Implications For Direct Detection Experimentsmentioning
confidence: 55%
See 1 more Smart Citation
“…In Figure 6, the approximate sensitivities to m χ = 5 GeV/c 2 DM are plotted as vertical lines to illustrate the potential cumulative effect the dark disk, density wake, and kinematic wake can have for various experiments (see [4,7,[73][74][75] for sensitivity determinations, where E R has been translated to v min as in Section III B). Each experiment has been able to place limits on σ χ and m χ , with the earlier generation CDMS-Si experiment [74] finding three possible events that make the most likely model for a DM particle m χ = 8.6 GeV/c 2 and σ χ = 1.9 × 10 −41 cm 2 , consistent with the CoGeNT results [4], as well as the DAMA (Na) results [5]. We also plot horizontal lines connecting the vertical line at m χ = 5 GeV (right extent) to a limit at m χ = 10 GeV (left extent) as a function of v min to demonstrate the different values of dR/dv min each experiment would reasonably expect to observe.…”
Section: B Implications For Direct Detection Experimentsmentioning
confidence: 55%
“…In the currently favored form of weakly interacting massive particle (WIMP) theory (see e.g. [1,2]), dark matter is composed of a single particle with a mass in the range of 10 GeV/c 2 , which a number of experiments are working to directly detect [3][4][5][6][7][8][9][10][11][12][13]. Direct-detection (DD) experiments seek to measure the weak nuclear recoils during elastic scattering between dark-matter (DM) particles and the nuclei of a target detector.…”
Section: Introductionmentioning
confidence: 99%
“…The solid, cyan lines represents the strategy outline by Eq. (27), where partial capture rates are defined along the diagonals as shown. The red (green) line represents the optical depth for hydrogen (helium).…”
Section: Appendix C: Generalized Multi-component Multiscattering Form...mentioning
confidence: 99%
“…(D5), where a double sum is performed over partial capture rates Cij. The solid, cyan lines represents the strategy outline by Eq (27),. where partial capture rates are defined along the diagonals as shown.…”
mentioning
confidence: 99%
“…1) The Gran Sasso Dark Matter (DAMA) experiment has seen an annual modulation in the event rate in its detector (44) with just the theoretical predicted form (45). The interpretation of this result is controversial, as other experiments have failed to detect dark matter and seem to be in contradiction with this detection claim (46,47).…”
Section: What Is the Dark Matter?mentioning
confidence: 99%