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CERN related research program in 2006-2011 Nuclear Physics. High energy nuclear physics ALICE experiment Installation and Commissioning Data taking Data analysis – offline computing Physics program HENP after 2011 Theory ISOLDE activity. ALICE at LHC. First collision: mid 2007
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CERN related research program in 2006-2011Nuclear Physics • High energy nuclear physics • ALICE experiment • Installation and Commissioning • Data taking • Data analysis – offline computing • Physics program • HENP after 2011 • Theory • ISOLDE activity
ALICE at LHC • First collision: mid 2007 • ALICE lifetime = 10 years
Installation and Commissioning – 2006 (1) • Installation of the TPC FEE • Dec. 2005 – Feb. 2006 • 3 people for 2 months 1 person-month @ CERN: ~35 kNOK
Installation and Commissioning – 2006 (2) • TPC/HLT pre-commissioningwith laser beams and cosmics • Feb. 2006 – Aug. 2006 • 1-2 people for 2-3 months • Installation of the TPC RCUs • Summer 2006 • 1 person for 2 weeks
Installation and Commissioning – 2006 (3) • Installation of the PHOS FEE and RCU • Spring 2006 • 2 people for 2 months • PHOS pre-commissioning and calibration • PS beam in summer 2006 for 8 weeks • 1-2 people for 2.5 months (shifts)
Commissioning - 2007 • Commissioning of the front-end electronics • TPC • PHOS • Installation and commissioning of the HLT • Full connectivity • 30% of computing power • First pp collisions in summer 2007 • First PbPb collision in 2008
Running scenario • First pp collisions in 2007 • 1 month per year heavy ion run • 7 months per year pp • Running schedule for the first 5 years • Regular pp runs at 14 GeVreduced luminosity between 1029and 5*1030 cm-2sec-1 which will leads to event rates from 10 kHz to 200 kHz • 2-3 years PbPb collisionsluminosity of 5*1026 cm-2sec-1 which leads to an interaction rate of 4 kHz • 1-2 years ArAr • 1 year pPb like collisions
Data analysis – offline computing • Scandinavian offline computing contributed through NDGF (Nordic Data Grid Facility) • Agreed sharing ATLAS/ALICE 50%/50% • ALICE computing needs approx. half of ATLAS but half the number of collaborators • LCG resource status: 50% shortfall for ALICE
ALICE ATLAS CMS HR 2001 LHCC 2004 HR 2001 LHCC 2004 HR 2001 LHCC 2004 Now Now Now CPU 16 26 35 17 41 65 26 40 55 Disk 2 9 13 3 21 24 4 14 26 MSS 5 11 11 20 11 11 10 16 17 Evolution of computing resources
Present status of pledged resources • Tier 0 at CERN • ALICE requirements satisfied, including peak for first pass reconstruction • Tier 1 and Tier 2 • As declared to LCG and presented to RRB • CAF not included
Physics program • Flow analysis (TPC, HLT) • High pt physics • Nuclear modification factor direct and 0, (PHOS, TPC, HLT) • Di-jets, gamma-jets (PHOS, TPC, HLT) • Heavy flavour • Open charm production (TPC, ITS, HLT) • production (TPC, TRD, HLT) • Ultraperipheral collisions (TPC, SPD+trigger detectors, HLT)
Nuclear Theory • Relativistic heavy ion collisions and quark-gluon plasma • Initial state • Final Freeze Out • Collective, Fluid Dynamical properties (“Third flow component”) • Phase transition dynamics
HENP after 2001 • ALICE running plan • pp or pp-like run at 5.5 TeV • Light AA system • dA • Low energy PbPb • Another high energy PbPb • ALICE upgrades ? • CBM at FAIR/GSI ? • Astrophysics experiment ?
108 106 104 102 100 M2 (GeV2) 10 GeV 10-6 10-4 10-2 100 x J/ψ ALICE at LHC – Phase 2 SHLC: shutdown (2012 ?) + upgrade 2012 - 2015 • Depending on physics results • Upgrades: detectors, FEE, DAQ, trigger • Example: detector covering large rapidities • Probe initial partonic state in a novel Bjorken-x range (10-3-10-6): • nuclear shadowing, • high-density saturated gluon distribution ALICE PPR CERN/LHCC 2003-049
CBM experiment at FAIR/GSI • Facility for Antiproton and heavy Ions Research • Planned commissioning: 2010 – 2015 • CBM experiment • super-dense baryonic matter • in-medium properties of hadrons
Dense Matter in the Universe • Mergers of binary stars – the ultimate nuclear collision • evolution depends on the equation-of-state of the matter inside the star • large differences between normal neutron stars and selfbound stars • different pattern of mass transfer • observable via gamma bursts, gravitational waves, ...? in 2020? astro/-ph/0403374
ISOLDE physics • Isotope Separator On-Line DEvice
Physics program • Experiments at REX-ISOLDE • Mass 80 region:Neutron-rich nuclei approaching the doubly closed shell nucleus 78Ni • Mass 132 region:important for r-process calculations • Mass 230 region:Coulomb excitation -> collective features • Nuclear shape • Multi-quasiparticle excitations • Detectors • Gamma arrays like MINIBALL • Compact disc detector for the scattered beam • Theory • Extreme, low-density nuclear states • Few– and many-body systems