From: Marc C Ross Sent: Tuesday, November 23, 2010 9:24 PM To: N.Toge; akira.yamamoto@kek.jp; carwar@fnal.gov; Victor R Kuchler; atsushi.enomoto@kek.jp; John.Andrew.Osborne@cern.ch; nicholas.walker@desy.de; peterg@fnal.gov; wilhelm.bialowons@desy.de; jmp@slac.stanford.edu Cc: Marc C Ross; Marc C Ross Subject: CFS / Global Webex meeting, Wednesday 24.11.2010; nominal time - PM report PAC review, 11-12 November, 2010 http://ilcagenda.linearcollider.org/conferenceTimeTable.py?confId=4680 Here are some highlights of the PAC review – from my notes: Michael Peskin’s talk was interesting – in it he explicitly referred to a higher energy for ILC. This is his last slide: “ The tight focus of the GDE on 500 GeV is a disadvantage in the debate over the correct energy. The question will always be raised: Can we eventually go to higher energies ? The GDE and its PAC should discuss a vision for later, higher energy stages of the ILC. This could play out over decades. A model is the “site-filler” accelerator vision in the original proposal for Fermilab. Mike Harrison discussed a staged approach to CLIC with ILC as the first stage. Another possible vision is a plasma wake-field accelerator (which could have the same time structure) as an afterburner to ILC. “ Here are some excerpts from my PAC closeout notes – (transcribed a week later). 1) The panel will strongly underline the fact that both Flash and Xfel are adequate SRF linac demonstrators. Another such demonstrator is not necessary. 2) It is essential that the core team be maintained post-2012. To keep the effort from diverging. 3) The committee was really impressed with SRF R&D progress. The recent results from JLab - 9 out of 10 testing successfully - is a tremendous achievement. With these results we have made the 'proof of principle' of the process; we now have to make it cheap. 4) The 9mA studies have made a further step forward. Having some time on Flash is not a contentious issue. 5) The DR extraction kicker studies have proven successful. Now the ATF team have to get the small beam size. 6) Cornell studies on e-cloud have been comprehensive and better than studies done anywhere else. Before the work stops it is important to benchmark the modeling codes. 7) SB2009. PAC was impressed with ongoing HLRF R&D at Slac and Kek. There is clearly much better collaboration with the physics community. 8) SRF industrialization. We have to preempt the XFEL costs. We have to be prepared to explain why the RF for ILC will not be just an extrapolation. LHC magnets could have been 2x or more expensive. But it turned out much better. We should follow the LHC example. Namely - to ask for the minimum required effort for each part. The PAC membership has ‘rotated’. Stuart Henderson, Hans Weise and Katsunobu Oide are new members. The written closeout draft will be sent to Barry and Sakue shortly. Then made public. Marc