NEWAGE -- A direction-sensitive dark matter search

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K. Miuchi NEWAGE -- A direction-sensitive dark matter search Kentaro Miuchi Kyoto University) H. Nishimura T. Tanimori, H. Kubo, S. Kabuki, K. Tsuchiya, A. Takada, Y. Okada, K. Hattori, K. Ueno, S. Kurosawa A. Takeda (ICRR), H. Sekiya (ICRR) (New generation WIMP search with an advanced gaseous tracker experiment)

description

NEWAGE -- A direction-sensitive dark matter search. ( Ne w generation W IMP search with an a dvanced g aseous tracker e xperiment). Kentaro Miuchi ( Kyoto University) H. Nishimura T. Tanimori, H. Kubo, S. Kabuki, K. Tsuchiya, A. Takada, Y. Okada, K. Hattori, K. Ueno, S. Kurosawa - PowerPoint PPT Presentation

Transcript of NEWAGE -- A direction-sensitive dark matter search

Page 1: NEWAGE  -- A direction-sensitive dark matter  search

K. Miuchi

NEWAGE -- A direction-sensitive dark matter   search

Kentaro Miuchi

( Kyoto University)H. Nishimura

T. Tanimori, H. Kubo,

S. Kabuki, K. Tsuchiya,

A. Takada, Y. Okada,

K. Hattori, K. Ueno, S. Kurosawa

A. Takeda (ICRR), H. Sekiya (ICRR)

(New generation WIMP search with an advanced gaseous tracker   experiment)

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K. Miuchi

OUTLINE

Direction sensitive DM search

Micro-TPC

NEWAGE surface run

FUTURE PLANS & SUMMARY

June11 2007   DBD07

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1 .   Direction sensitive DM search    “ WIMP-wind” detection

The WIMP-wind

WIMPV0 =230 km/s

SOLAR SYSTEM220 km/s

PLB 578 (2004) 241

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WHY “Direction-sensitive” ?Large mass for exclusion ( and indication )

BUT Annual modulation is not enough…

Direction-sensitive for detection

WIMPWIMP WIND WIND γ γ

FF

Annualmodulation

direction

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Sensitivities Goal: Detect the WIMP-wind  ( 2010~ )

• underground ・ low pressure ( CF4 0.05 bar ) ・large volume ( 1m3 × N )

CURRENT: • surface ・ CF4 0.2 atm ・ 30cm cube

sensitivity

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2 micro-TPC (3D tracking device)

Feb. 20, 2007   APPEAL07

Position Encoder

PIC (×5000)

GEM(×10)

TPC

Particle tracks

e

Preprints: physics/0701085 K.Miuchi et.al

40cm

TPC

X readout ( 768ch ) Y

readout ( 768ch )

FAGA position encoder( 1536ch )

23×28×31cm3

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-PIC (gas gain 5000)• 400mm pitch• 589824 pixels• 768+768 readout

2D imaging device

28cm

23cm

30cm μPIC(Toshiba)

Large area GEM(scienergy)

Takada et. Al. PSD7

PIC

GEM

TPC 30cm

5mm

Particle tracks

e

GEM (gas gain 10)

140mm pitch

70mm diameter

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Readout electronics• 768 anode + 768 cathode• Digital (LVDS) signals at ASD• (X,Y,T) at the position encoder

    for tracking

Feb. 20, 2007   APPEAL07

31cm

gas volume

Kubo et. al. IEEE/NSS 2005

TPC system

ENCODER

ASD

for energy

+ Summed analog signal

TPC   systemGas volume

• DRIFT length 31cm• CF4 0.2bar gas

100MHz, pipeline

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CF4+C4H10 (9:1) 0.2 atm

n -> p forward scattering (emulation of WIMP -> F scatterings)

Jan 27, 2007   3rd MPGD workshopRecoil direction  image

252Cf( NE45°  zenith35° )

10

Cos

n

p

CF4+C4H10

252Cf run

Proton tracks

n252Cf

YX-15cm

15cm

15cm

-15cm

30cm

Z(drift)

0cm

TPC performance 1:           nuclear tracks, imaging

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TPC performance 2:   gamma-ray rejection

energy   length   correlation

gamma-rays from 137Cs

neutron ( BG )

neutron ( BG )

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  gamma-ray rejection ( continued )spectrum, BG subtrucction

• gamma rejection <  2e-4  ( statistics limited )

neutron ( BG )

Subtracted energy spectrumEnergy spectrum

thick: 137Cs run

hatched: no source

consistent with 0 ( >100keV )

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K. Miuchi June 11, 2007   DBD07

TPC performance: nuclear track efficiencyneutrons from 252Cf

• 0.4 @ 100keV

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Surface run①2006 Nov.1st ~ Nov.27th

exposure 0.15 kg days (=0.0089kg ×16.7days)

@Kyoto university (N35.03   E135.783 ) Energy spectrum ( conventional method )

Energy spectrum

3 Surface run

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Surface run ②The sky map (by nuclear recoil tracks)

flat neutron background is seen

North sky view seen by C and F nuclei(100-400keV)

DM direction

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Jan 27, 2007   3rd MPGD workshop

Surface run ③Cosθ distribution

consistent with a flat distribution

Cosθ 分布

(100-400keV)

DM limit

First step to theNEWAGE

WE ARE   HERE

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K. Miuchi Jan 27, 2007   3rd MPGD workshop

Go   undergroundJUST   started

KAMIOKA LAB-B2006/12/12

KAMIOKA LAB-B2007/1/19

Osaka

KyotoKamioka

4 Next step…

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SUMMARYμTPC : 30cm cube in operation

direction-sensitive method works!

NEWAGE : underground run just started

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20062006 年年 1111 月月 1717 日日

TPC performance ②  stability

Drift velocity: fast drop

⇒ slow decrease after 1 day

gain, energy resolution :  stable within   the systematic error

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エネルギー校正• ガラスに蒸着した 10B   ( 厚さ 0.6μm )• ドリフトケージ内部にセット、外から 252Cf の中性子を減速して照射• 10B(n,a)7Li 反応  (Q=2.70MeV 1.8MeV for )• 原子核による校正、低エネルギーへの線形性は別途確認示す必要あり• 現状では、校正には 6 時間程度、見せれる絵には 12 時間程度かかって

いる

XY イメージ

keV

スペクトル

エネルギー vs 飛跡長

keV

Li

2000

スペクトル(GEANT4 )

検出器応答

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位置分解能から角度分解能• アルファ線の飛跡を直線フィット、残差を求める: 0.8mm• BG run の C,F recoil での 飛跡長 / (nhit-1) = 1mm   ( サンプリング密

度 )

• 上記二つのパラメータをもちいてsimulation 振る。

• NHIT=3  で直線 FIT すると左の様になる。

• ローレンツィアンで FIT して、 γ=25°(=HWHM)

検出器応答

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エネルギー分解能• 高エネルギー( 5-8MeV )ではラドンのピークを使ってモニタ• 40 % FWHM• これは検出器固有の数字(ゲインのばらつきが効いている)

• 低エネルギーでは、以前の Ar での実測 60 % FWHM@60keV• これが電子数統計とすると、

W 値、エネルギーで外挿すると、 60×sqrt((54/26)×(60/100))   =   70 % FWHM   @100keV

60%@59.5keV

検出器応答

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Gas gains • operation gain for MIPs ~50,000

Gain curves

Gain map

Gain uniformity • Maximum / minimum = 2.2

TPC   performance (with Ar+C2H6 gas)

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K. Miuchi June 11, 2007   DBD07

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TPC performance①   tracking400m digital “HIT” ( for tracking) + summed analog ( for energy)

F 500keV 5~6mm    in 0.2atm CF4

F,C tracks

n

252Cf

YX-15cm15cm

15cm

-15cm

30cm

Z(drift)

0cm

X,Y image Z projection

Fidutial   24×21.5×31cm3

(CF4 8.9g)FLAT response

trigger

Trigger :z=0

cm 30

Preprints: physics/070118 K.Miuchi et.al

• gamma rejection <  2e-4  ( statistics limited )

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データ シミュレーション

クロスセクション

検出器の方向依存感度マップ

測定値

「 DM の風」

測定値

×

sim

=

sim

Expected 「 DM の風」

sim

Expected cosθ 分布( DM )

Input: エネルギー分解能、角度分解能、

WIMP 質量、エネルギー BIN

Input: エネルギー BIN 、絶対検出効率

For given   WIMP 質量、

反跳エネルギー

WIMP 質量、エネルギーBIN

ごとに用意

比較

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Jan 27, 2007   3rd MPGD workshop

SpectraSpectra• Energy spectra from the whole volume

   (with energy corrections)

109Cd

linearity

Energy resolution

133Ba

241Am

Ag-KCu-K

Cs-KCu-K

Cu-K

59.5keV

60%@59.5keV

22.2+24.9keV

31keV

8keV

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Jan 27, 2007   3rd MPGD workshop

Particle TrackingParticle Tracking muons

Electrons (~100keV)

Protons (~2MeV)

30cm

Neutrons( 252Cf )

511keV   ‘ s( 22Na )

Cosmic ray muons

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Jan 27, 2007   3rd MPGD workshop

3D Spatial resolution3D Spatial resolution• Fit muon tracks with straight lines• plot the residuals

Residual muon tracks

dataFitted line

data

residual

Residual (short drift)

Residual (long drift)

)2

exp(2

222 rr

22222 )( lDdetectordiffusiondetector

Drif

t le

ngth

-PIC

mm1

mm2

mm51.0detector

cmmm/37.0D

)2

exp(2

222 rr

dependence on drift length

r [cm] 

r [cm] 

l [cm]