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Project SIMPLE for Dark matter

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The Group

FRANCE PORTUGAL USA

H. S. Miley (PNNL)

G. Waysand (CNRS) T. A. Girard (CFN)

J. I. Collar (Chicago)

D. Limagne (CNRS) T. Morlat (CFN)

F. Giuliani (CFN)

M. Felizardo (CFN/ITN)

A. R. Ramos (CFN/ITN)

J. G. Marques (CFN/ITN)

The search for Dark Matter

Cold Dark Matter

Dark Energy : 67  6 % 29  4 %

inference from galaxy

supernovae observations dynamics









~30% ~70%





baryons : 4  1 %

direct observation,

  m    1

inference from

elemental abundances

m  l   B   NB

~1% ~4%

~25%

Dark Mater candidate:

Neutralino

→ Lagrangian : elastic scattering of a generic WIMP (spin ½) on nucleon :

32 J 1

A  G 2  A  (a p  S p  an  S n ) 2

2





f

J

Target = ?



Spin dependent channel





L  4 2GF     (a p p   p  an n  n)     ( g p p  p  g n n n) 

Spin INdependent channel





4

A  GF  A  ( g p Z  g n N ) 2  A2

2 2





Target = heavy atom

Spin dependent channel









→ Cross section (limite) would reach a maximum, depending on

(Ref. Tovey et al, PLB 488 (2000) 17):

p2

1

*Proton sensitive:  lim A

 lim



 A CA / C p

p A 2 p

(WIMP independent model)

J 1

C A ,n / C p ,n  4 / 3

p

 S p ,n  2

J



n2

1

*Neutron sensitive:  lim A

 lim



 A CA / C p

n A 2 n

(WIMP independent model)

To detect the beast

Xe, Ge

Requirements:

(neutron sensitive)

→ Cross section max in the spin dependent :



Fluorine

(proton sensitive)







→ Cross section max in the spin Independent: Heavy atom Target (Xe, I…)





→ Detector with low recoil energy 1-100 KeV





→ Problem of background for direct detection:

Low rate of event ~ 30 μm)



→ Matrix (food products):

• Gelatine (1.8%) :

pig skin and not bones: low content in Ca & K

• Bidistilled water (16%)

• Polyvinylpyrrolidone PVP (3.6%) :

to decrease solubility of freon

• Glycerine (78.6%) :

matching density, high mouillability (no spurious

event on the walls)

Purification of the matrix



Purification of food products: well known in the food industry.

Purification of the ingredients with M+ MP500 Lewatit resin for

metal extraction (anionic exchange resins).

Filtration system with acropack filter 0,2 microm.

→ radiocontamination 0.5 then sensitive to

X-rays, α-rays and cosmics

ray muons.



Installation of the SDDs inside

the pool

Results of 0.42 kgd exposure

(42 g @ 10 day)



Ref: T. A. Girard et al, PLB 621 (2005) 233









 p Cp

2



 lim A   A

lim



 A CA

p 2 p







From experiment





Main background:

*Leaks from the cap ~ 30/kgd

*Neutrons < 3/kgd

*Alpha < 0.5/kgd

*radon < 1/kgd

A     p

A

n

A  2

lim

A  A ,n  4GF  AC A ,n

p 2 2 p







Ref: T. A. Girard et al, PLB 621 (2005) 233





+

 p ,n C p ,n

2



 lim A

 lim



 A C A ,n

p ,n A 2 p









2

 a  

 p



an  

  lim ( A)  n  A

lim  24 GF  p

2 2

 p 





aP  a p an  an

2 2

Near futur:

Tasks for nov 2006 (3kgd)





Improvements to do, from the last experiment (0.42kgd):

 short exposure (10d) : increase the lifetime of the SDD, how?









 Leak : resolve the leak problem from the caps : change the

“Mc Gyver cap” into something more professional





 Acoustic, reduce the electronic background noise

Increase the lifetime, how ?





 Droplet: by recompression



 Interface droplet-matrix : surfactant as shielding against

Oswald ripening effect

droplet too small+ possibility of foam = loss of efficiency







 Matrix: additives - increase the fracture energy ?

Delayed the formation of fractures

Fracture experiment









Refs: Y. Tanaka et al, Eur. J. Phys. E 3 (2000) 395

T. Morlat et al, NIMA 560 (2006) 339

Result with additives

T. Morlat et al, NIMA 560 (2006) 339









PEG: no because of crystallisation of the glycerine

Agarose: increase resistance to fracture + Shift the

Tsol-gel

Leaks from the cap ?









BEFORE

NOT ANYMORE !!!

The solution









AFTER

The sound acquisition for nov 2006









1







0.5







0









(V)

Piezoelectric Preamplifier Data -0.5



Noise: 100-200mV Transducer Acquisition

-1







-1.5

0.022 0.023 0.024 0.025 0.026 0.027 0.028 0.029 0.03 0.031

(s)





Test in Rustrel : background noise down to 0.95mV

BEFORE

AFTER

What we expect for the 3kgd

(nov. 2006)





Agarose to increase the time of exposure (40 days)





New cap: no leaks in 3 weeks under presure





New electronic with low background noise





7 “fresh SDDs” (~80 g), fabrication in Rustrel (no transportation)

New limit projected

Heavy project: Cf3I (ρ=2g.cm-3)

for Spin-INdependent sector

The impact of a CF3I SDD

gp N

 0

gn Z







Z N:









Z N:

gp gn 

(  )2 

 p ( A)

SI

 nSI ( A) 4GF  p

2 2

CF3I feasible ?



The non matching density: few preliminary calculs:

    

 f  0  f visc  p  0 ρ0, η

D 4 ρb

6r   ( b   0 )r 3 g  0 D

t 3

2r 2 gt ( b   0 )



9D



2(35 .10 6 ) 2 9.81(60 x60 )( 2.10 3  1.3.10 3 )

AN   

9 x5.10  2

  0.13 kg.m 1s 1





 The following composition gives ηexp=0.17 kg.m-1.s-1

(measured by a viscosimeter Cannon Fenske routine 1600-6400):



gelatine (1.71%)+ PVP (4.18%)+ biH2O (15.48%)+ agarose (0.46%) + glycerine (78.16%).

CF3I :

temperamental





 High solubility under presure : S=0.5g/kg H2O/bar

 High solubility at T
 No stockage at T<0°C: clathrates of hydrates









1 night at 7ºC









Day 0 Day 1



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