beyond counting: directional approach to dark matter detection

31
Beyond Counting: Directional Approach to Dark Matter Detection Denis Dujmic, MIT for DMTPC Collaboration Miami 2008, Dec 18

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Page 1: Beyond Counting: Directional Approach to Dark Matter Detection

Be

yo

nd

Co

un

tin

g:

Dir

ectio

na

l

Ap

pro

ach

to

Da

rk M

att

er

De

tectio

n

Denis

Dujm

ic, M

ITfo

r D

MT

PC

Co

llab

ora

tio

n

Mia

mi 2008, D

ec 1

8

Page 2: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

8,

20

08

Mia

mi 2

00

82

/31

Da

rk M

att

er

Ha

lo

(8.5

kp

c)

Page 3: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

8,

20

08

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mi 2

00

83

/31

WIM

P

Win

d

Sp

erg

el, P

hys.R

ev.

D3

7 (

19

88

) 1

35

3

<v>

~2

20

km

/s

z

x

z

x

00

:00

12

:00

Diu

rnal variation in W

IMP

direction:

Page 4: Beyond Counting: Directional Approach to Dark Matter Detection

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08

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mi 2

00

84

/31

Dir

ectio

na

lity

Recoil

angle

(10

0G

eV

WIM

P o

n f

luo

rin

e)

F

���

F

Str

ong forw

ard

-backw

ard

asym

metr

y

in r

ecoil

angle

Page 5: Beyond Counting: Directional Approach to Dark Matter Detection

De

c 1

8,

20

08

Mia

mi 2

00

85

/31

He

ad

-Ta

ilW

ithout head-t

ail

Backgro

und

(iso

tro

pic

)

With h

ead-t

ail

Page 6: Beyond Counting: Directional Approach to Dark Matter Detection

De

c 1

8,

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08

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mi 2

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86

/31

WIM

P S

ea

rch

es

Spin

independent

Spin

dependent

Page 7: Beyond Counting: Directional Approach to Dark Matter Detection

De

c 1

8,

20

08

Mia

mi 2

00

87

/31

Is L

arg

e

Exp

osu

re

En

ou

gh

?v~

220km

/s

Decem

ber

June

Gala

ctic p

lane

Pre

fere

ntial

WIM

P d

irection

R. B

ern

ab

ei e

t a

l.,

Eu

r.P

hys.J

.C5

6:3

33

-35

5,2

00

8

DA

MA

/LIB

RA

1-2

% v

aria

tio

n in

co

un

tin

g r

ate

with

exp

ecte

d p

erio

dic

ity

an

d p

ha

se

!

WIM

P w

ind?

Page 8: Beyond Counting: Directional Approach to Dark Matter Detection

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08

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/31

Dir

ectio

n-S

en

sitiv

e S

ea

rch

Go

als

•C

orr

ela

te W

IMP

sig

nal w

ith a

str

ophysic

al

phenom

ena -

unam

big

uous s

ignal

dete

ction

•S

ensitiv

ity to s

pin

-dependent in

tera

ctions

•G

ood r

eje

ction o

f backgro

unds

•S

cala

ble

to larg

e v

olu

mes

Page 9: Beyond Counting: Directional Approach to Dark Matter Detection

De

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20

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89

/31

Co

nce

pt

of

Dir

ectio

na

l

De

tecto

r

FE

e-

e-

e-

e-

drift

reg

ion

Am

plif

ication

regio

n

+

V-V

‘Head

‘Tail’

~2

mm

- D

MT

PC

, A

hle

n,

Fis

he

r e

t a

l. (

20

04

)

- N

EW

AG

E,

Ta

nim

ori

et

al. P

LB

57

8 (

20

04

)

- M

IMA

C-H

e3

, S

an

tos e

t a

l (2

00

0)

- D

RIF

T,

Mar

toff

et a

l., N

IMA

440

(20

00)

- B

uckla

nd

, L

eh

ne

r,M

ase

k,M

oja

ve

r, P

RL

73

(1

99

4)

Low

-

pre

ssure

gas

Page 10: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

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20

08

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mi 2

00

81

0/3

1

DM

TP

C

Co

llab

ora

tio

n

R. V

ande

rspe

k

A. P

iso

J. M

onro

eG

. Sci

olla

A. K

abot

hR

. Yam

amot

o

D. D

ujm

icB

. Cor

nell

W. F

edus

P. F

ishe

rH

. Yeg

orya

n

J. L

opez

T. S

ahin

A. L

ee

S. H

ende

rson

S. A

hlen

A. R

occa

ro

H. T

omita

K. O

tis

H.

Wel

lens

tein

F. G

olub

S. G

oyal

Page 11: Beyond Counting: Directional Approach to Dark Matter Detection

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1/3

1

“Da

rk

Ma

tte

r

TP

C”

Fe

-e

-

-V

Charg

e

readout

Lig

ht re

adout

CC

D (

PM

T)

Lig

ht re

adout

CC

D (

PM

T)

-V0V

+V

0V

10-liter

pro

toty

pe

Ta

rge

t:

CF

4 g

as

�2J(J

+1

)~0

.65

~5

0T

orr

Page 12: Beyond Counting: Directional Approach to Dark Matter Detection

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2/3

1

Mesh E

lectr

odes

for

Charg

e

Am

plif

ication

G1

0

SS

rin

g

SS

rin

gR

esis

tive

se

pa

rato

rs

dia

=0

.5m

m,

eve

ry 2

cm

e-

e-

SS

or

Cu

me

sh

D.Dujmic

et

al.,A

str

op

art

.Ph

ys.3

0:5

8-6

4,2

00

Page 13: Beyond Counting: Directional Approach to Dark Matter Detection

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3/3

1

Op

tica

l re

ad

ou

t

20

0 3

00

40

0 5

00

60

0 7

00

80

0 (

nm

)

He

+C

F4

(40

%)

Ar+

CF

4

(5%

)

Ar+

CF

4

(67

%)

CF

4

M.M.F.R. Fraga et al. NIM A 504 (2003) 88

A.Kaboth et al. NIM A 592 (2008) 63

Scin

tilla

tion in C

F4:

CC

D Q

E

(KA

F0

40

1M

E)

CF

4+

e- �

(C

F3

+)*

+ F

+ 2

e- ’

CF

4+

+ e

- �

(C

F4

+)*

+ 3

e- ’

Well

matc

hed w

ith C

CD

QE

:

�/e

- ~

1/3

(1

50-8

00nm

)

Page 14: Beyond Counting: Directional Approach to Dark Matter Detection

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mi 2

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4/3

1

Ch

arg

e R

ea

do

ut

Readout of entire

mesh (

one c

hannel)

Test w

ith 5

.9keV

x-r

ay s

ourc

e (

Fe55):

Charg

e g

ain

:

�E

/E~

19%

D.D

ujm

ic e

t a

l.,

ICH

EP

08

pro

ce

ed

ing

s, a

rXiv

:08

10

.27

69

Energ

y r

esolu

tion@

5.9

keV

:

M =

e�

d >

10

5

Page 15: Beyond Counting: Directional Approach to Dark Matter Detection

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20

08

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mi 2

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81

5/3

1

Constr

uction

(Sum

mer/

Fall

2008)

H.Y

eg

ori

an

, M

IT

T.

Co

ldw

ell,

MIT

Page 16: Beyond Counting: Directional Approach to Dark Matter Detection

De

c 1

8,

20

08

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mi 2

00

81

6/3

1

r

E

r

E

150V

/cm

Dri

ft C

ag

e FE

M c

alc

ula

tio

n

of

fie

ld u

nifo

rmity

~2

0cm

(lim

ited b

y

ele

ctr

on

diffu

sio

n)

~2

0cm

Page 17: Beyond Counting: Directional Approach to Dark Matter Detection

De

c 1

8,

20

08

Mia

mi 2

00

81

7/3

1

>90cm

Page 18: Beyond Counting: Directional Approach to Dark Matter Detection

De

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08

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81

8/3

1

Ca

libra

tio

n w

ith

Alp

ha

So

urc

e

15.5

cm

15.5

cm

100T

orr

241A

m

5.5

MeV

alp

ha fro

m241A

m

dE

dx

10cm

- E

nerg

y, ra

nge

calib

ration

- U

niform

ity

Page 19: Beyond Counting: Directional Approach to Dark Matter Detection

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9/3

1

Exp

osu

re t

o N

eu

tro

n B

ea

m Neutr

ons

from

252C

f

WIM

Ps

• C

an w

e s

ee n

ucle

ar

recoils

?

• R

econstr

uct direction?

• S

ense o

f direction?

• G

am

ma r

eje

ction?

Page 20: Beyond Counting: Directional Approach to Dark Matter Detection

De

c 1

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20

08

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mi 2

00

82

0/3

1

Typ

ica

l R

eco

il Im

ag

es

neutr

ons

5m

m

Page 21: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

8,

20

08

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mi 2

00

82

1/3

1

Ima

ge

An

aly

sis

- E

nerg

y fro

m v

isib

le lig

ht

- R

ange fro

m s

pan o

f

recoil

track

- 2D

angle

- H

ead-t

ail

from

lig

ht

asym

metr

y

Neutr

on

direction

Page 22: Beyond Counting: Directional Approach to Dark Matter Detection

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2/3

1

En

erg

y-R

an

ge

Nucle

ar

recoil

band

Energ

y d

istr

ibution

Energ

y-r

ange

Good a

gre

em

ent w

ith S

RIM

sim

ula

tion

Page 23: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

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08

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3/3

1

Ga

mm

a R

eje

ctio

n

F (

~1m

m, 5

0keV

)

e- (~

30m

m, 1

5keV

)

>10

6

(usin

g C

s-1

37 s

ourc

e)

e-

C F

Tim

ur

Sa

hin

, M

IT,

GE

AN

T4

,

50

To

rr C

F4

e-

�B

ased o

n d

iffe

rence in s

toppin

g p

ow

er

(Diffe

rent ra

nge for

sam

e e

nerg

y!)

Page 24: Beyond Counting: Directional Approach to Dark Matter Detection

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08

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4/3

1

“He

ad

-Ta

il”D

irection s

ense (

head-t

ail)

fro

m lig

ht asym

metr

y

First dem

onstr

ation b

y D

MT

PC

!

Sig

ne

d c

osin

e o

f

2D

re

co

il a

ng

le

Cf-

25

2,

75

To

rr C

F4

2D

an

gle

+ h

ea

d-t

ail

fro

m lig

ht

asym

me

try

Re

so

lutio

n (

de

g)

Neutr

on

direction

D.D

ujm

ic e

t a

l., A

str

op

art

. P

hys.

30

(2

00

8)

58

D.D

ujm

ic e

t a

l., N

ucl. I

nstr

. M

eth

A5

84

(2

00

8)

32

7

Page 25: Beyond Counting: Directional Approach to Dark Matter Detection

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mi 2

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5/3

1

“He

ad

-Ta

il” Quality

� HT<

0 c

orr

ect head-t

ail

� HT�0

wro

ng h

ead-t

ail

Quantify

asym

metr

y

with s

kew

ness:

�HT=

x�x

()3

x�x

()2

3/2

Head-t

ail

Qualit

y:

QHT=��1�2�f w

rong

()2

Err

or

on a

sym

metr

y ~

(Q

HT)-

1/2

Cf-

25

2,

75

To

rr C

F4

Page 26: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

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20

08

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mi 2

00

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6/3

1

10

-lite

r P

roto

typ

e

Su

mm

ary

• T

akin

g d

ata

in b

asem

ent at M

IT

• E

xperience w

ith c

ontinuous r

unnin

g

• B

ackgro

und r

ate

, ty

pes

• F

irst re

sults w

inte

r 2009

• E

xpect best lim

it fro

m a

directional

dete

cto

r

Page 27: Beyond Counting: Directional Approach to Dark Matter Detection

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7/3

1

Ne

xt

ste

p:

1m

3 d

ete

cto

r

• 4�2

5cm

dri

ft v

olu

me

s

• C

CD

� E

MC

CD

• tr

anspare

nt anode

CC

D

PM

T

Charg

e r

eadout

PM

T

CC

D

1m

1.2

m

Dra

win

g:

H W

elle

nste

in,

Bra

nd

eis

Page 28: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

8,

20

08

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mi 2

00

82

8/3

1

1 m

3

100 m

3

SD

couplin

g

Plo

t: G

.Scio

lla,

MIT

Page 29: Beyond Counting: Directional Approach to Dark Matter Detection

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c 1

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20

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9/3

1

100

m

20

m

Prop

osed D

US

EL c

avern

CM

S:

15 x

15

x 2

2 m

3

SN

O:

21

x 2

1 x 3

4 m

3

Sup

er-K

:

40

x 4

0 x

40

m3

DM

TPC

:

16 x

16

x 1

6 m

3

1 to

n C

F4

@5

0T

orr

Page 30: Beyond Counting: Directional Approach to Dark Matter Detection

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0/3

1

• 1

kg o

r m

ore

(1-1

0m

3)

• 1

-5 y

• W

IPP

(2000 f

t)

• W

inte

r/S

pring 2

009

• 1

ton o

r m

ore

(>

1000s m

3)

• 5

-10y

• D

US

EL (

4850ft o

r 7400ft)

Un

de

rgro

un

d

Site

s

Page 31: Beyond Counting: Directional Approach to Dark Matter Detection

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1/3

1

Dis

co

ve

ry o

f w

ind

: [e

.g.

Mo

rga

n,

Gre

en

20

07

]

10

s e

ve

nts

(w

ith

HT

)

10

0s e

ve

nts

(w

/o H

T)

Dir

ectio

na

l A

pp

roa

ch

to

Da

rk

Ma

tte

r D

ete

ctio

n

U

nd

ers

tan

din

g D

M h

alo

[e

.g.

Ge

lmin

i,

Go

nd

olo

20

01

; M

org

an

, G

ree

n,

Sp

oo

ne

r 2

00

5]

10

0s (

str

ea

ms?

)

1,0

00

s (

sp

he

rica

l h

alo

?)

10

,00

0s (

ha

lo s

tud

y)

Astr

onom

y P

hase

Dis

covery

Phase

- D

em

onstr

ate

d d

ete

cto

r concept

- C

urr

ently takin

g d

ata

with 1

0L d

ete

cto

r

(surf

ace)

- M

ove

to

WIP

P in

Win

ter/

Sp

rin

g 2

00

9

- C

onstr

uction o

f 1m

3 dete

cto

r (2

009)