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Laboratoire Souterrain de Modane Past present future

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Title: Laboratoire Souterrain de Modane Past present future


1
Laboratoire Souterrain de Modane Past -
present - future
  • Gilles Gerbier
  • CEA/LSM

2
COMMISSARIAT À LÉNERGIE ATOMIQUE
DIRECTION DES SCIENCES DE LA MATIÈRE
3
1984-1988 Fréjus Proton Lifetime  DVP  900 tons
of Fe geigers tubes plasma tubes
4
The lab now
  • 1750 rock above
  • 4800 mwe
  • Dry and warm (32 )
  • 4 muons /m2/ day
  • 1 .6 10-6 fast neutrons/cm2/s from
  • rock/concrete radioactivity
  • air continuously renewed 1.5 vol/hour
  • very low Rn concentration 5-15 Bq/ m3

5
NEMO 3 bb expt with 100Mo IN2P3, Dubna, Moscou,
Prague
Mo 2?2? results 2004
6
NEMO3 january 2005
7
Hunting for galactic dark matter WIMPs
EDELWEISS II Start installation jan 2005 Data
taking autumn 2005 w. 28 detectors (9
kg) Upgrade possible up to 36 kg
10 layers of 12 detectors of 320 g
EDELWEISS-I present
EDELWEISS-II sensitivity goal
1 Ton sensitivity goal (optimistic)
July 6 2002 -GG
8
(No Transcript)
9
Super Heavy elements In Nature Dubna CSNSM
expt Ekaosmium (Z 108, A 286) Detecting decay
by multi neutron evt from Os sample in neutron
detector with 60 3He counters Goal Sensitivity
10-22 g/g
Installed at LSM since 2004
10
Germaniums 13 detectors (unique world wide)
for low level radioactive counting
Bordeaux wine dating with 137Cs
11
About 150 physicists, engineers, techs from
enlarged Europe come to LSM few from US and
Japan
Project of joint laboratory with Dubna
JOULE JOint Undergroung Lab in Europe
LSM
12
The EU Deep Underground Labs
13
Team in Modane
Running the lab people
Safety control
Partially in Modane
Chargé mission MégT Luigi Mosca
Sécurité DAPNIA Alain Le Saux
Sécurité IN2P3 Cyril Thieffry
Charlotte Riccio
14
New safety galery
SFTRF digs new galery start 2006 end 2009
New excavation ??
Projets
15
Mid 2009 the two digging machines meet at LSM
location gtpossibility of 15 000 m3 extension
Safety galery
Actual lab 3 500 m3 Full
15 m
Extension 15 000 m3
Road Tunnel
Benefits of infrastruture for digging and
excavating Little impact on total excavation (lt 7
) gt low cost
16
What for ?
  • NB 15 000 m3 40 of 1 Gran Sasso hall
    1.5 of Megaton cavity
  • Well adapted for
  • Third generation bb and dark matter WIMP searches
    (100 kg to 1T) looking for deep sites
  •  Small  size neutrino detectors
  • Dedicated low level radioactive environment
    (integrated neutron shield/m veto, radon reduced
    atmosphere)
  • SuperNemo bb (10 000 m3), Eureca DM (2 000 m3),
    neutrino coherent detection (1 000 m3), LXe,

17
Infrastructures in Modane town offices,
garage/storage, appartment
18
Conclusion
  • New physics results in coming 5-7 years
  • New generation experiments coming on-line
  • Local infrastructure ready to welcome ambitious
    program
  • Welcome to the afternoon visits
  • Welcome back for physics together in few years
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