1. WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)

2. WIMP ( Weakly Interacting Massive Particle) search One of the strong candidates of dark matter,introduced from the supersymmetry theory Interacting rarely -> Below 1 cpd (count/kg/keV) Expected recoil energy to the target nucleus -> a few keV - a few tens keV By measuring nuclear recoil energy, We can observe WIMP scattering.

3. KIMS’ WIMP search tool -> CsI(Tl) crystal scintillator High light yield : ~60000 photons / MeV Easy fabrication & Handling Easy to have the large mass with an affordable cost,enabling study of seasonal variation of WIMP interaction Better Pulse Shape Discrimination than NaI(Tl) Sensitive to spin dependent and independent interaction of WIMP both -> Complementary to other pioneering Spin independent WIMP Search (CDMS, Xenon-10)

4. CsI crystal detectors & data collected CsI(Tl) Crystal 8x8x30 cm 3 (8.7 kg) x 4 3” PMT (9269QA) : Quartz window, RbCs photo cathode ~5 Photo-electron/keV Crystalp.e./keVMass (kg) Data (kg·days) S0501A4.68.71147 S0501B4.5 8.71030 B0510A5.9 8.7616 B0510B5.9 8.7616 Total 34.83409

5. Neutron calibration 300 mCi Am/Be source  a few 100 neutrons/sec hit 3cm  3cm  3cm crystal (sample)  Quenching factor of Recoil Energy Nuclear Recoil mean time distribution NeutronsampleGamma Full size Gammasample Tag γ(4.4MeV) to measure TOF and energy of neutrons

6. PMT data without crystal PMT noise significantly limits the sensitivity at the low energy range. PMT only data taken ~350 kg days for each crystal with the PMTs used for each crystal to understand the PMT noise event Clean acryl box PMT

7. PMT data without crystal WIMP search data PMT only data

8. Event selection Likelihood fit with F(t) = 1/τ f exp(-(t-t 0 )/τ f )+r/ τ s exp(-(t-t 0 )/τ s ) Gamma Neutron PMT only (dot-dashed) WIMP search DATA

9. Event selection Gamma PMT only (dot-dashed) WIMP search DATA Asymmetry = (PMT1 –PMT2)/total PMT 3-5keV 5-7keV

10. Event selection coincidence cut spectrum of the sum of energy of all the crystals

11. Effect of cuts on MT distribution DataGamma Neutron PMT Log(MT) distribution at various cut stage

12. Selected Events WIMP search Data after cutWIMP search Data after efficiency correction

13. Extraction of Nuclear Recoil event Fit the WIMP search data with PDF function from gamma and neutron calibration data  extract NR events rate Neutron calibration gamma calibration

14. Extraction of Nuclear Recoil event Estimated nuclear recoil rates

15. WIMP Nucleus Cross section Assuming WIMP forms a spherical halo around our galaxy. has a Maxwellian velocity distribution. -> Interaction rate of WIMP with the target nucleus (according to WIMP mass & Cross-section) Cs I WIMP density ρ D =0.3 GeV/c 2 /cm 3 Earth’s velocity v 0 =220km/s Local galactic escape velocity v esc =650km/s σ WIMP-p = 7.2x10 -6 pb WIMP Mass = 50 GeV

16. Simulation of expected energy spectrum Fix σ WIMP-p = 7.2x10 -6 pb, WIMP Mass = 50 GeV Cs I GEANT4 Simulation considering Quenching factor, Energy resolution, form factor, detector character

17. Limit on WIMP nucleus cross section 90% CL Central value

18. WIMP Nucleus Cross section Scalar: Spin independent interaction -> coherent amplification via constituent nucleon Axial: Spin dependent interaction -> coupling depends on proton & neutron spin expectation value

19. Spin independent limits Nuclear recoil of 127 I of DAMA signal region is ruled out. WIMP density ρ D =0.3 GeV/c 2 /cm 3 Earth’s velocity v 0 =220km/s Local galactic escape velocity v esc =650km/s PRL 99, 091301 (2007)

20. Spin dependent limits Pure proton case Pure neutron case PRL 99, 091301 (2007)

21. New results using 3409 kg days data Published in PRL 99, 091301 (2007) DAMA signal region is ruled out for both SD and SI Interactions at WIMP mass > 20 GeV World best limit on SD interactions for pure proton case New results using 3409 kg days data Published in PRL 99, 091301 (2007) DAMA signal region is ruled out for both SD and SI Interactions at WIMP mass > 20 GeV World best limit on SD interactions for pure proton case Conclusion of this data analysis

22. 12 crystals(104.4kg) installed. 1 st Calibration run was over. Started data taking. 12 crystals(104.4kg) installed. 1 st Calibration run was over. Started data taking. Current status

23. Current background level cpd (count/kg/day) keV 2-3 cpd

24. 12 full size crystals(8x8x30cm 3 ) ~ 100 kg installed ->Current shielding can accommodate 250 kg. Data taking was started. Internal backgrounds reduced to 2cpd level. After 1-2 year operation, Annual modulation of WIMP wind can be studied. 12 full size crystals(8x8x30cm 3 ) ~ 100 kg installed ->Current shielding can accommodate 250 kg. Data taking was started. Internal backgrounds reduced to 2cpd level. After 1-2 year operation, Annual modulation of WIMP wind can be studied. prospect