1. 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

2. 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

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

4. 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

5. 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

6. 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

7. 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

8. 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

9. 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

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

11. 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

12. 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

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

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

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

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

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

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

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

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

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

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

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

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

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