Diapositive 1

1
France with two institutions CEA/DSM/Dapnia,
CNRS/IN2P3.
2
Research Ministery
I
CERN
CEA
CNRSUniv
IN2P3 (20 labs,2600p)
DSM
GIE GANIL
APC
DAPNIA (750p)
LSM
CC LYON
SPhN
SPP

IRES
LAL
IPNO
CPPM

Figure 1
3
IN2P3 and DAPNIA

• IN2P3
• Mission for CNRS plus universities in nuclear and
  particle physics
• 20 laboratories in 15 different universities
• 1000 permanent scientists (1/2 CNRS, 1/2
  universities), 1500 IT CNRS, 300 non permanent
  2800
• DAPNIA
• Particle, nuclear and astrophysics
• Location Saclay
• 635 permanent plus about 130 non permanent 770

4
French Nuclear and High Energy Physics Budget

• CERN 100 Meuros
• CNRS Universities 200 Meuros (3/4 for salaries)
• CEA 55 Meuros (3/5 for salaries)

5
Distribution of activities

• IN2P3
• 1/4 Quarks and charged leptons
• 1/4 Nuclear Physics
• 1/4 Astroparticle physics plus neutrinos
• 1/4 Accelerator RD plus instrumentation RD plus
  interdisciplinary activities (including nuclear
  energy)
• DAPNIA
• 1/4 particle physics
• 1/4 astrophysics (not included in the 55 Meuros
  CEA)
• 1/8 nuclear physics
• 1/4 accelerator RD plus instrumentation RD
• 1/8 interdisciplinary activities

6
French Roadmap for HEP and Astroparticle

• A Bottom-Up approach involving the whole French
  scientific community.
• Coordinated by a steering committee composed of
  members from the scientific committees of DAPNIA
  the IN2P3.
• A workshop on the future of nuclear and high
  energy physics was held from the 6th to the 10th
  October 2004 at la Colle-sur-Loup and gathered
  together more than 400 researchers,
  teacher-researchers and engineers.
• The management of the CEA-DAPNIA and the
  CNRS-IN2P3 have distilled the summary given in
  the document  from Quarks to Cosmos .

http//council-strategygroup.web.cern.ch/council-s
trategygroup/
7
The Ultimate Constituents of Matter
CMS Solenoid
Objective 1 Fully exploit the potential of the
programmes in progress at FNAL, SLAC DESY.
Objective 2 Fulfil our commitments to the LHC
experiments ATLAS and CMS , LHCb construction
and installation of the detectors, preparation of
the analyses, start-up of the detectors in 2007.
8
The Ultimate Constituents of Matter
Objective 3 From 2007, ensure an optimal
exploitation of the physics potential offered by
the LHC and its detectors, and prepare a possible
accelerator upgrade.
L 1035 cm-2 s-1 ??
9
The Ultimate Constituents of Matter
Objective 4 Take part in the accelerator RD in
the CLIC project (CTF3). Take part in the
accelerator RD and the design of a detector for
the ILC.
CLIC Cavity
Cold tuning system
Fast piezoelectric actuator
Integrated cavity RF tests in CryHoLab
10
The Ultimate Constituents of Matter
Understand the structure of nucleons (partons
distributions, spin) and, more generally, or
hadrons (COMPASS at CERN, TJNAF 6-12 GeV, FAIR at
GSI), by both experimental and theoretical
efforts
TJNAF
Micromegas _at_ COMPASS
11
Neutrinos, Astroparticle and Cosmology
Objective 1 Ensure the success of the current
large projects AUGER, HESS, ANTARES, VIRGO,
GLAST, AMS, PLANCK, NEMO, OPERA, T2K. Objective 2
Continue neutrino astronomy, with a 1 km3
underwater telescope in the Mediterranean sea at
the 2010 horizon. An improvement of HESS is
envisaged (HESS II) in the 3-4 years to come.
SN G347.3-0.5 g (0.8-10 TeV) et X
12
Neutrinos, Astroparticle and Cosmology
Objective 3 VIRGO Detector for the detection of
gravitational waves , now in commissioning, will
reach its maximum of sensitivity in the two
coming years. R D in progress could lead to a
follow-up of VIRGO for the detection of the
gravitational waves (Around 2010 2015)
Objective 4 Modernisation and expansion of the
underground laboratory of Modane within an
international framework, in order to house
detectors permitting the study of proton
stability, to detect supernovae and to study
neutrino properties with CERN beams (Around
2015-2020)
13
Neutrinos, Astroparticle and Cosmology

• Objective 5 Space is another very important
  priority axis. The experiments under construction
  will have to be carried through ( PLANCK GLAST
  horizon 2007, AMS one to two years later), the
  new generation of experiments in cosmology and
  gravitation (JDEM/DUNE, LISA, around 2012-2013)
  and also the study of cosmic phenomena of high
  energy (SIMBOL-X and ECLAIRS horizon 2008-12)
  will have to be prepared.

14
Neutrinos, Astroparticle and Cosmology
Objective 6 Follow-up the experiments on cosmic
rays of the highest energy (collaboration AUGER
in Argentina), dark matter research (EDELWEISS
with Modane) and neutrinoless double beta decay
researches (SUPERNEMO)
EDELWEISS
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EXTREME STATES OF NUCLEAR MATTER
Ensure in the next few years a maximum
exploitation of the physics potential offered by
PHENIX and STAR experiments of RHIC. Complete
ALICE construction at LHC (2007), and starting in
2008, exploit its strong scientific potential
during ten years.
PHENIX _at_ RHIC
ALICE _at_ CERN/LHC
16
SCIENTIFIC COMPUTATION

• Objective 1 Reinforce the calculation resources
  of the computing centre IN2P3/DAPNIA of Lyon
  within the framework of the LHC Computing Grid
  project
• Objective 2 Relay this action at the regional
  or inter-regional level by the creation of
  computation poles inserted in the grid.

17
ACCELERATORS and INSTRUMENTATION

• Objective 1 Continue the R D on the high
  gradient superconducting accelerating cavities
  and the power couplers (ILC, EURISOL), together
  with intense protons sources and intense heavy
  ions sources (gt 1mA).
• Objective 2 Take part with the CERN in the RD
  on CLIC in preparation of a 5 TeV e e- linear
  collider at CERN around 2020.
• .

Drive beam - 180 A, 70 ns from 2.4 GeV to 240 MeV
with -9MV/m
QUAD
QUAD
POWER EXTRACTION AND TRANSFER
STRUCTURE (PETS)
ACCELERATING
30
GHz
- 150 MW
STRUCTURES
Main beam 1.5 A, 58 ns from 9 GeV to 1.5 TeV
with 150MV/m
BPM
CLIC UNIT
(6000 modules at 3 TeV)
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ACCELERATORS and INSTRUMENTATION

• Objective 3 Build a high intensity proton
  injector for CERN (IPHI) in order to increase the
  intensity of the machines at CERN (LINAC4
  project) and be prepared for intense neutrinos
  beams or radioactive heavy ions beams (SPL
  project) at CERN, possibly coupled with EURISOL
  (beta beams, around 2015-2020)...
• Objective 4 Continue innovating technical RD
  in acceleration technique, in particular laser
  driven accelerators.
• Objective 5 Research on innovating detection
  technologies.

IPHI SPIRAL2 RFQ
Micromegas for T2K and ILC