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Welcome in the Paris Sud Campus Welcome to LAL
Achille Stocchi LAL director Professor at the Paris-Sud University
21th November 2013
Welcome in the Paris Sud Campus Welcome to LAL Achille Stocchi LAL - - PowerPoint PPT Presentation
Welcome in the Paris Sud Campus Welcome to LAL Achille Stocchi LAL director Professor at the Paris-Sud University 1 21 th November 2013 1 Personnel ~ 2000 The Site where you are Superficies ~ 100000m 2 The Labs : CSNSM, IAS, IMNC, IPNO,
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Welcome in the Paris Sud Campus Welcome to LAL
Achille Stocchi LAL director Professor at the Paris-Sud University
21th November 2013
Site - Polytechnique Site – ParisSud/Vallée Site – CEA/Ormes de Merisiers Site – CEA/Saclay IRFU IRFU CSNSM, IAS, IMNC IPNO, LAL, LPT LLR
The Site where you are
The Labs : CSNSM, IAS, IMNC, IPNO, IRFU, LAL, LLR, LPT
Labs grouped under P2IO label and belonging to 4 agencies : Paris Sud, CNRS, CEA and Ecole Polytechnique
Personnel ~ 2000 Superficies ~ 100000m2
Le Plateau La Vallée
1500 m
60% national community
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This Pole of the Physique des deux Infinis et des Origines (P2IO) groups laboratories situated in the Orsay Campus :
de Masse (CSNSM), UPS-CNRS,
et Cancérologie (IMNC), UPS-CNRS,
And on the Plateau:
(IRFU) - site CEA,
CNRS, - campus de l’Ecole Polytechnique
Nuclear Physics, Interdisciplinary , Cosmology/Origins Astrophysics and Cosmology/Origins Medical Physics : Imaging and Radiotherapy Nuclear Physics, Hadronic, Astroparticles Particles, Astroparticles and Cosmology Theoretical Physics Nuclear, Particles, Astroparticles and Cosmology Particles, Astroparticles and Cosmology
www.lal.in2p3.fr
Laboratoire de l’Accélérateur Linéaire (LAL) (IN2P3/CNRS and Paris Sud University)
Biggest CNRS HEP laboratory in France: ~120 physicists ~220 engineers/technicians Annual budget ~10 Meuros + ~20MEuros (salary) Hosting ~10-15 PhD thesis / year Historical name: big linear e+e- accelerator was stopped in 2004. Instead new facilities have been built (see later) Surface of 18 000 m2, including 7 000 m2 of halls, workshops and clean rooms Located at the Paris Sud University campus between Orsay and Bures-sur-Yvette
www.lal.in2p3.fr
Laboratoire de l’Accélérateur Linéaire (LAL) (IN2P3/CNRS and Paris Sud University)
Biggest CNRS HEP laboratory in France: ~120 physicists ~220 engineers/technicians Annual budget ~10 Meuros + ~20MEuros (salary) Hosting ~10-15 PhD thesis / year Historical name: big linear e+e- accelerator was stopped in 2004. Instead new facilities have been built (see later) Surface of 18 000 m2, including 7 000 m2 of halls, workshops and clean rooms Located at the Paris Sud University campus between Orsay and Bures-sur-Yvette
Few example of experimental Program at LAL
Main projet: LHC at CERN
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ATLAS frontal view LHCb side view
Nobel Prize 2013
Example of other projects
Experiments on accelerators : BaBar, D, H1 Planck satellite Auger Observatory and JEM/EUSO for cosmic rays at ultra high energy Studies of neutrino physics with the NEMO detectors. Direct search for gravitational wave using the interferometer Virgo Accelerators : XFEL in Germany, PHIL at LAL, ATF/ATF2 in Japon…. (see later)
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Prix Nobel 2008
Implications in future projects
Next generation of electron-position linear colliders Projets ILC and CliC Futur telescopes LSST LHC upgrades !
Couplers : assure the transmission of the HF-waves from (klystrons) to supraconductives cavities
XFEL
Projet of ~ 20 MEuros (Thales)
Serie production 640 (XFEL) et 30 (ILC) COUPLERS 1.3GHz
Very high flux of X-rays produced form accelerated electrons sent on ondulators. XFEL is installed at DESY-Hambourg Projet – Couplers at LAL
(IRFU responsible of the cryomodule)
Production is now lunched ! (visit after the morning session)
Compton back-scattering Electron beam of 50 MeV laser amplified with a Fabry-Perot cavity
~2015 first interactions
Collaboration : CELIA, C2RMF,LAL, NEEL, SOLEIL,THALES, ESRF, INSERM, UPS,UB1.
LAL leads the project EQUIPEX Project =12MEuros
In the main domain of expertise LAL participates to a European bid for and e/g facility in Roumanie ELI-NP. Projet ~66Meuros (our part ~20MEuros) {Thales, Amplitude, Alysom…). Collaboration Italo-franch-britannic
Compact Source of X-rays( 50-90 KeV) At high flux(~1012 ph/s)
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Projet « IGLEX » :
In the same place two (for the moment) platforms unique based on innovative concepts in terms of photons and ions sources for pluiridisciplinary searches
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Andromède is a new instrument for the mass spectrometry analyses of nano-objects
Information is got from the impact of nanoparticles accelerated by a Van de Graaff from 1 to 4 MV and analyzed by microscope at electronic or protonic emission
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Today électrons at 3 MeV@5Hz, Q ~ 100 pC Ambitious program for using PHIL as a detector facilty. Work in progress
gradient ~ 90 MV/m - 2011
ps pulse, emittance 5 µm.rad – 2013 BPM strip line – 2013 – for THOMX
top Hat spatial – 2013 laser 100 fs - ?
News : transfert arm to change photocathode. collaboration CTF (CLIC-CTF)
gluons to nucleons and nuclei
~ 360 members ~22000 m2 ~ 30 MEuros/year including salaries ~ 130 publications/year
A pillar of nuclear physics research and Accelerator technology in Europe
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Heavy Ion Collisions at LHC
strong interaction: (de)confinement, chiral symmetry breaking (restoration)
primordial Universe (few μsec after the Big Bang)quark-hadron
A major player in understanding hadrons and hadronic matter
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major player in Pierre Auger Observatory
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TANDEM: 15 MV Van de Graaff 50 MeV e-Linac On line isotope separator
SIHL TARGET LAB Thin Target Lab IS Lab
2 HR spectrometers
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A major Player in Accelerator design and technology
SPIRAL2 superconducting Cavity assembly (in white room)
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A major player in Accelerator design (few examples)
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The SUPRATECH Platform @ IPNO
see talk Sébastien Bousson/Jean-Luc Biarrotte
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Impacting research activities with state of the art instrumentation
MUST 1&2 AUGER G0 DVCS AGATA
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e
Detector to be tested Magnet with adjustable field Collimator 1 Collimator2
Sample of “monochromatic” electrons Variable energy ~100 keV and 5 MeV adjustable intensity 104 electrons ~1 fC … LEETECH :– Platform for testing detector @PHIL
µ 2 m
Hodoscope 1 : MRPC
détecteurs à testerHodoscope 2 : MRPC
µ 2 m
First run beginning 2014
First run Summer 2014
Three “common” PLATEFORMES to test detectors are in preparation
Captinnov : platform P2I0 for innovative captors
To characterize the circuits and the detectors in prototyping or pre-production phases Integrating hybrids systems (det/PCB/electronics) with large density of channels and/or large dimensions
Bonding Machine
@ LAL @ IRFU
CORTO:COsmic Ray Telescope @ Orsay
CSNSM, IAS, IMNC, IPNO, IRFU, LAL, LLR, LPT LAL, IPNO LAL
Centre de Sciences Nucléaires et de Sciences de la Matière Research fields
Nuclear physics Nuclear Astrophysics Solid State Astrophysics Solid State Physics Chemical Physics of Irradiation
A total of 110 people including 40 researchers and 30 post.doc. and Ph.D. Highly interdisciplinary Annual budget ~2 Meuros + ~8 MEuros (salary)
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CSNSM PROJECTS
“Masses of exotic calcium isotopes pin down nuclear forces”, Nature. “Plumbing Neutron Stars to New Depths with the Binding Energy
“UltraCarbonaceous Antarctic micrometeorites, probing the solar system beyond the nitrogen snow-line”, Icarus, 04/2013, article dans “Le Monde”
"hidden-order" in URu2Si2 », PRL by Bareille… and A. F. Santander "Faisabilité de la formation de nanoprécipités d'oxyde par implantation ionique dans des aciers Fe-10%Cr : application au cas de matériaux nucléaires pour les réacteurs nucléaires du futur".
Ce Zheng, Aurélie Gentils, Joël Ribis, Odile Kaïtasov, Vladimir A. Borodin, The feasibility of Al-based oxide precipitation in
Fe-10%Cr alloy by ion implantation, submitted to Phil. Mag. (Sept. 2013)
Few Highlights
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Some example of “original” CSNSM activities
NUCLEAR ASTROPHYSICS. Primordial and stellar nucleosyntesis, low energy cosmic rays in the Galactic region… SOLID STATE ASTROPHYSICS Discovery of ultracarboneous Antarctic micrometeorites (UCAMMs) in the CONCORDIA Collection of CSNSM New campaign of Micrometeorites in Antarctic at Dome C
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ARAMIS Accélérateur de 2MV IRMA Ions implanter
Plateforme JANNuS
Large chioce of implementation parameters Pratically all the elements from Pratiquement He to Bi . Ions energy from 10 keV to 5 MeV Sample’s Température from liqiud azote (-196 °C) to 1300°C
Experimental set up
Caracterisation line: structure, stœchiometry, composition Implementation line : syntesis of new Material , doping
② brain metabolism :
➜ neurons-astrocytes cross-talknetworks :
➜ olfactory – feeding crosstalk⑤ modelling of biological systems
➜ dynamical systems research ➜ oncological systems modeling : tumor growth...Imaging & Modelling for Neurosciences & Cancerology laboratory
(IMNC - UMR 8165)
① in vivo small animal imaging :
➜ wide field optical imaging (intrinsic, hyperspectral...) ➜ b+ probes for freely moving intracerebral imaging③ imaging probes for radioguided surgery
➜ compact and hand held gamma imaging ➜ optical imaging endogenous fluorescence④ PET/SPECT quantitation
➜ tomographic reconstruction ➜ estimation of physiol. parameters
radiotherapy
➜ mini beams ➜ hadrontherapy
technical services
modelling for life sciences
IMNC 2.0 : the « Health » interface of the P2IO Valley project
Biology Diagnostic Therapy
Imaging Instrumentation Modelling Simulation Biology Methodologies
Interface of Physics- Cancerology Upstream Physics
➜ Photodetection ➜ Micro-electronics ➜ Accelerators (THOMX) ➜ Theoritical Physics ➜ Simulation & Modelling ➜ CPU & DM (Virtual Data)
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LAL IPN LPT
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Health
➜ Clinical imaging ➜ Small animal imaging ➜ Protontherapy ➜ Mini-beams ➜ Dosimetry ➜ Radiobiology
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UPSay labs (P2IO, PHOM…) Paris Diderot labs UPSay Physics Medicine Cluster Paris CHU
SHFJ IR4M Curie CPO
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solaire stellaire système solaire Cos, MI
astrochimie
exoplanètes
COROT
Planck
Mars Express
Cassini
ROSETTA
Stardust
BepiColombo ExoMars
Herschel
Solar Orbiter
Hayabusa 2
Technical Teams
“station d’étalonnage”
Spica ?
Euclid
Echo / Plato
JUICE
SPACE Projets
SOHO /Golf (1995) Solar Seismology
Solar Images at 4 wavelengths as got from in 2012 by EIT / SOHO, operating since 1995
Examples of space experiences
Planck/HFI
« Station d’étalonnage » for testing space instruments
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New DATA Center of about 300m2 in construction grouping 8 laboratories :
net infrastructure
With :
« Virtual Data » CENTER
Preliminary phase almost concluded ! 100m2 / 400KW IT / 30 racks, cost ~ 1M€ with a new room here close by in the Valley Final Phase 250m2 / 1,5MW / 84 racks Toal Cost : 3M€ CSNSM, IAS, IMNC, IPNO, IRFU, LAL, LLR, LPT Actual situation 650 m2 of informatics room within 8 labs fragmented in more than 10 rooms (from 25 à 100 m2) hosting 900 KW Very inefficient and expensive (1 M€/an)
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CSNSM Facilities
TEM
(transmission electron microscope)
Spectrometer SIDONIE (isotopically pure targets)
2 MV TANDEM/VdG 185 kV implanter
Recherche et Technologie à l’IAS
Micro-caméras
Développement d’une chaîne de détection pour la qualification de systèmes de micro-imagerie visible de nouvelle génération
Compression
Développement d’un ASIC de compression de donnée par ondelette
Roue à filtres
Développement d’une roue à filtres compacte pour Solar orbiter
Filtres UV
Filtres métalliques minces pour FSI / Solar orbiter
DSI Echoes
Développement d’un interféromètre de type Max-Zhender
Matrices de bolomètres
DCMB (développement concerté de matrices de bolomètres), CUBIC
Filtres Bayer
Filtre de Bayer spatialisable pour détecteur matriciel
de 3 à 5 M€ par an de contrats industriels
Compétences - Prestations
Plateforme JANNuS
Expérience des interactions avec les industriels
(3S Photonics, IIIV Labs)
Prestations régulières dans le domaine du spatial (gage de fiabilité)
l’INTA (Espagne).