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Direction-sensitive dark matter search with MPGD

Direction-sensitive dark matter search with MPGD. NEWAGE experiment. MPGD2011@Maiko 2011/08/30. Kiseki Nakamura (Kyoto university). T.Tanimori , K.Kubo , K.Miuchi , T.Mizumoto , J.Parker , A.Takada , H.Nishimura , S.Iwaki , T.Sawano , Y.Matsuoka , S.Komura , Y.Sato. Dark Matter

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Direction-sensitive dark matter search with MPGD

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  1. Direction-sensitive dark matter search • with MPGD NEWAGE experiment MPGD2011@Maiko2011/08/30 Kiseki Nakamura (Kyoto university) T.Tanimori, K.Kubo, K.Miuchi, T.Mizumoto, J.Parker, A.Takada, H.Nishimura, S.Iwaki, T.Sawano, Y.Matsuoka, S.Komura, Y.Sato • Dark Matter • Direction-sensitive search • NEWAGE Detector "m-TPC" • Low pressure gas • Summary

  2. Dark Matter (DM) • Rotation curve of stars in the galaxy does not dump even outer region • ⇒ DM at galaxy • Observation of cosmological parameters • ⇒ DM at cosmological scale • ⇒ Unknown mass "Dark Matter" exist at various scale 200 Rotation curve energy fraction of space MNRAS 249 (1991) 523 observed Rotation velocity of stars [km/s] 100 DM baryon gas 0 Distance from GC[pc] 0 10 20 30 WMAP/NASA

  3. DM candidate "WIMP" Weakly Interacting Massive Particle • DM candidates • WIMP • axion • sterile neutrino • Q-ball • ...etc • neutralino (c) • Lightest neutral SUSY particle • It can be WIMP • Elastic scatter with nucleus Super Symmetry theory DM Schematic image of elastic scattering Standard model particles and SUSY particles nucleus We observe recoil nucleus neutralino consists of these particles

  4. DM detection method 1 • 1. Annual modulation (conventional) • Large mass->Solid or liquid detector • Require for 3s : ~10000events • 2. Incoming direction of DM (new) • Nuclear track->Gas detector • Require for 3s : ~20events Expected energy spectrum 2 σSD=1pb M=100GeV target:F rate [counts/keV/kg/days] 1 Few % of the annual modulation Annual modulation observed by DAMA 0 100 200 0 recoil energy [keV]

  5. DM detection method 2 • 1. Annual modulation (conventional) • Large mass->Solid or liquid detector • Require for 3s : ~10000events • 2. Incoming direction of DM (new) • Nuclear track->Gas detector • Require for 3s : ~20events Expected cosθ distribution σSD=1pb M=100GeV target:F Large difference in forward to back DM θ Nucleus cosq

  6. Direction-sensitive DM search DRIFT [UK] NEWAGE [Japan] 30cm • MWPC (2mm pitch) • First started direction-sensitive method • Underground • Low background • Large size (1m3) • m-PIC (400mm pitch) • Only NEWAGE obtained direction-sensitive limit • Underground 1m 10cm 25cm • CCD • 2D image • Identification of head-tail • Reading to underground • Micromegas (~400mm pitch) • Measured quenching factor in detail • R&D at surface DMTPC [USA] MIMAC [France]

  7. MPGD advantages for DM search • Direction sensitivity • Detect short track • ( Typically 2mm@100keV(F in 0.1atm CF4) • Background decrease • Discriminate electron tracks (BG) from nuclear tracks by track length • ( rejection : 10-6 ) Energy-length relation (by 137Cs) electron events MPGD(u-PIC) Energy-length relation (by 252Cf) 400mm

  8. NEWAGE

  9. NEWAGE Detector "m-TPC" New general WIMP search with an Advanced Gaseous tracker Experiment • m-TPC • gas : CF4 • pressure : 0.1-0.2atm 0.5cm 30cm or 50cm • GEM (8-segmented) • size : 28x23cm • thickness : 50mm • hole : 70mm • pitch : 140mm • m-PIC • size : 30x30cm • pitch : 400mm Drift plane 30cm

  10. Data taking Track 1. ASD (Amp Shaper Discriminator) See which strip hit 2. Position Encoder (100MHz) Take coincidence (drift field : 625 V/cm/atm) (drift velocity : 8.5 cm/ms) Energy Flash ADC (100MHz) (*) 65cm ASD m-TPC 45cm 45cm Flash ADC Position Encoder (*) IEEE Tra. Nuc. Sci. 51, 4, 1, Aug. 2004, 1337-1342

  11. NEWAGE up to 2010 PLB 686 (2010) 11 • Place : Kamioka (depth : 2700m.w.e) • Exposure : 0.524 [kg days] • Pressure : 0.2atm • cosq distribution : Flat • Limit : 5600pb for 150GeV

  12. Next • We aim to search DAMA-region (sensitivity x1000) • Background: 1/10 ( x10) • ->Radon elimination (sub talk) • Material selection • Energy threshold: 1/2 ( x10) • ->low pressure gas (main talk) • Large size ( x10) • ->Several 1m3size detectors • ( current : (30cm)3 ) • Head-tail identification ( x3) • -> New DAQ (time-over-threshold) Expected limit curve of the WIMP-proton SD elastic scattering cross section (90%C.L.) PLB686 (2010) 11

  13. Gas circulation system Detector wall • Circulation with cooled charcoal • Radon rate : 1/4(prototype pump) • Futher reduction is expected with full spec (600ml/min) pump Detection region (76torr CF4) U Rn Rn a-decay (about 6MeV) Time dependence of Rn cooler 210K pump 20ml/min without circulation charcoal 160g 　　・ spiral:60g ・ cylinder:100g with circulation

  14. Low Pressure Experiments

  15. How to make threshold lower Expected energy spectrum Energy threshold : 100keV -> 50keV -> Sensitivity to DM : x10 σ=1pb, M=100GeV, target:F new threshold (plan) • Low pressure gas(152torr ->76torr) • ->Track length: x2 • Advantage • Sensitive to low energy (short) tracks • Improve angular resolution • Difficulty • Electrons density : half • ->Necessary gas gain : x2 (=1500) current threshold

  16. Drift Plane Gain curves Drift -3.69kV • m-TPC works at 0.1atm gas • Gain curve • anode ( m-PIC amplification ) • DGEM ( GEM amplification ) • induction ( passing rate ) GEMtop -500V GEM GEMbottom -280V Induction 5mm cathode GND m-PIC anode 515V gas gain gas gain gas gain GEM:-500/-280V anode:515V GEMbottom:-280V anode:515V DGEM:220V 2 times gain from 0.2atm DGEM=GEMtop-GEMbottom EInduction=GEMbottom/5mm anode voltage[V] DGEM voltage[V] Einduction(Induction field)[V/mm] • Gain curves saturated ( mean free path of e- : several mm ) • Reach the sufficient gain derived from 0.2atm operation

  17. Angular resolution • Compare the cosq distribution between measured to simulation (simulate each angular resolution) • We checked 50-100keV range : 40[deg] • (Can't be seen at 0.2atm) F nucleus tracks 252Cf Simulated cosqdistribution (400-800keV) cosq distribution (400-800keV) angular resolution 252Cf Blue:measured Green:simulation(s=49deg) neutron Blue : This work (0.1atm) Red : Previous (0.2atm) q nuclear

  18. Detection efficiency Expected energy spectrum • Detection efficiency : 0.6@50keV • (ratio of measured to simulation) • Energy threshold : 100 -> 50keV angular resolution σ=1pb, M=100GeV, target:F new threshold (plan) current threshold detection efficiency

  19. Summary • NEWAGE • Dark Matter search with MPDG "u-TPC" • u-TPC can detect Incoming direction of DM • Low pressure (152torr⇒76torr) • Operation test • u-PIC work at 76torr with sufficient gain • Angular resolution • 40°+3.1-2.9@50-100keV • Detection efficiency • 0.6@50keV • Energy threshold : 100 -> 50keV • Next to search DAMA • Update gas circulation system for radon elimination • Use new DAQ for head-tail identification • Simulation for constructing thelarge size detector

  20. Summary Thank you for your attention! • NEWAGE • Dark Matter search with MPDG "u-TPC" • u-TPC can detect Incoming direction of DM • Low pressure (152torr⇒76torr) • Operation test • u-PIC work at 76torr with sufficient gain • Angular resolution • 40°+3.1-2.9@50-100keV • Detection efficiency • 0.6@50keV • Energy threshold : 100 -> 50keV • Next to search DAMA • Update gas circulation system for radon elimination • Use new DAQ for head-tail identification • Simulation for constructing thelarge size detector Mascotof NEWAGE "Daakumatan"

  21. まだだ、まだ終わらんよ

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