Marcello A. Giorgi Università di Pisa & INFN Pisa Project outlook Marcello A. Giorgi Università di Pisa & INFN Pisa Annecy- XII General Meeting March16-19, 2010 3/19/2010 M.A.Giorgi

On process We have been visited by President of INFN No showstopper in the approval process Slightly slower than we expected CIPE is examining the proposal for a full funding O(700 M€) PNR insertion expected soon with highest priority would allow a special funding from the MIUR from national Research Undivided Fund. 3/19/2010 M.A.Giorgi

On process Mou for TDR agreed between INFN and IN2P3. Mou’s circulated to: 3/19/2010 M.A.Giorgi

On process Mou for TDR agreed between INFN and IN2P3. Mou’s circulated to: SLAC Canada BINP – to Siberian section of the Russian Academy of Science. 3/19/2010 M.A.Giorgi

On process Mou for TDR agreed between INFN and IN2P3. Mou’s circulated to: SLAC Canada BINP – to Siberian section of the Russian Academy of Science. Bilateral agreement between INFN and Spain is ready. 3/19/2010 M.A.Giorgi

People The convention between INFN and IN2P3 for making possible hiring people in LAL that can work for example in Frascati within LNF Accelerator Division had received in a positive way by INFN. Still not in operation. Management is working to accelerate timing. 3/19/2010 M.A.Giorgi

This meeting Good progress in the preparation of white paper: Physics document ready Detector and Accelerator in a good shape expected soon. Geometry working group has done a very good job for the best possible design of the detector. We all acknowledge the positive response by the community. 3/19/2010 M.A.Giorgi

We have now flexibility in parameters for the “baseline luminosity 1036” we have also a parameter list for low c.m.s.Energy runs 3/19/2010 M.A.Giorgi

Parameters Tau/charm threshold running at 1035 Baseline + other 2 options: Lower y-emittance Higher currents (twice bunches) Baseline: Higher emittance due to IBS Asymmetric beam currents RF power includes SR and HOM

Some personal whishes.. Physics studies to continue evaluating any special request to detector. Some examples: 3/19/2010 M.A.Giorgi

Some personal whishes.. Physics studies to continue evaluating any special request to detector. Some examples: Impact of polarization on physics discovery still not sufficiently elucidated. It must be also connected to possible requests on detector design. 3/19/2010 M.A.Giorgi

Some personal whishes.. Physics studies to continue evaluating any special request to detector. Some examples: Impact of polarization on physics discovery still not sufficiently elucidated. It must be also connected to possible requests on detector design. Charm studies need more effort also in view of decisions about forward PID 3/19/2010 M.A.Giorgi

Structure of Web page is there Present version 3/19/2010 M.A.Giorgi

Structure of Web page is there Present version Will soon become 3/19/2010 M.A.Giorgi

Structure of Web page is there Present version Will soon become So far it is empty! 3/19/2010 M.A.Giorgi

Next time in Elba for our meeting XIII May 31-June 4, 2010 3/19/2010 M.A.Giorgi

http://agenda.infn.it/conferenceDisplay.py?confId=2262

Tentative schedule Meeting: May 31 – June 4 Departure 1st arrival Opening plenary 2nd arrival Det Board Accel Board Project Board Detector parallel sessions

Thank you to: 3/19/2010 M.A.Giorgi

Thank you to: Director of Lapp 3/19/2010 M.A.Giorgi

Thank you to: Director of Lapp Yannis 3/19/2010 M.A.Giorgi

Very special Thanks to: 3/19/2010 M.A.Giorgi

Very special Thanks to: Andrea 3/19/2010 M.A.Giorgi

Very special Thanks to: Andrea, Myriam 3/19/2010 M.A.Giorgi

Very special Thanks to: Andrea, Myriam and to 3/19/2010 M.A.Giorgi

Very special Thanks to: Andrea, Myriam and to Lucia 3/19/2010 M.A.Giorgi