Limits on WIMP-nucleon cross section with CsI(Tl) crystal detectors
By H. Lee, H. Bhang, J. Choi, H. Dao, I. Hahn, M. Hwang, S. W. Jung, W. Kang, D. Kim, H. Kim and 18 more. 2007
183 citations recorded by the source corpus.
The Korea Invisible Mass Search(KIMS) experiment presents new limits on WIMP-nucleon cross section using the data from an exposure of 3409 kgd taken with low background CsI(Tl) crystals at Yangyang underground laboratory. The most stringent limit on the spin dependent interaction for pure proton case is obtained. The DAMA signal region for both spin independent and spin dependent interactions for the WIMP mass higher than 20 GeV/c^2are excluded by the single experiment with crystal scintillators.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/f7602621508679066f303856b2c12914b1695f5e
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In Nuclear and High Energy Physics
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Citations in the corpus
- AN INDIRECT SEARCH FOR WEAKLY INTERACTING MASSIVE PARTICLES IN THE SUN USING 3109.6 DAYS OF UPWARD-GOING MUONS IN SUPER-KAMIOKANDE (2011, unknown): “Also shown are results from direct detection experiments: DAMA/LIBRA allowed region (Savage et al. 2009), KIMS (Lee et al. 2007), and PICASSO (Archambault et al. 2009); and from neutrino telescopes: AMANDA (Braum et al. 2009) and IceCube (Abbasi et al. 2009).”
- Dark matter direct detection with non-Maxwellian velocity structure (2009, result): “Recent studies [26, 28, 43, 44] have shown that iDM remains a viable explanation of the DAMA data, consistent with recent results from CDMS [45], XENON10 [46], KIMS [47], ZEPLIN II [48], ZEPLIN III [49] and CRESST [50].”
- Global interpretation of direct Dark Matter searches after CDMS-II results (2009, methodology): “The KIMS experiment has an exposure of 3409 kg days taken with low background CsI(Tl) crystals [16].”
- Dark Matter Candidates from Particle Physics and Methods of Detection (2010, background): “At the moment, the leading direct detection experiments, such as CDMS, COUPP, and KIMS, are less promising in terms of probing the heart of supersymmetric and UED WIMP parameter space, as seen in Figs.”