Long term life time and future of the STAR TPC
Present at the meeting(s) were: myself (Jerome Lauret), Alexei Lebedev, Yuri Fisyak, Jim Thomas, Howard Wiemann, Blair Stringfellow, Tonko Ljubicic, Gene van Buren, Nikolai Smirnof, Wayne Betts (If I forgot anyone, let me know).
It is noteworthy to mention that the TPC future was initially addressed at the Yale workshop in (Workshop on STAR Near Term Upgrades) where Gene van Buren gave a presentation on TPC - status of calibration, space charge studies, life time issues. While the summary was positive (new method for calibration etc...) the track density and appearance of new distorsions as the lumisoity ramped up remained a concern. As a reminder, we include here a graph of the initial Roser luminosity projection.
which was build from the following data2002 | 2003 | 2004 | 2005 | 2006 | 2007 | 2008 | 2009 | 2010 | 2011 | 2012 | 2013 | 2014 | |
Peak Au Luminosity | 4 | 12 | 16 | 24 | 32 | 32 | 32 | 32 | 32 | 48 | 65 | 83 | 83 |
Average Au Store Luminosity | 1 | 3 | 4 | 6 | 8 | 8 | 8 | 8 | 16 | 32 | 55 | 80 | 80 |
Total Au ions/ring [10^10] | 4 | 8 | 10 | 11 | 12 | 12 | 12 | 12 | 12 | 12 | 12 | 12 | 12 |
An update summary of the status of the TPC was given by Jim Thomas at our February
2005 collaboration meeting (A brief look at the future evolution of TPC
track distortions ; see attachement below) to adress ongoing GridLeak
issues. Slide 19 summary for teh future is added here:
Will the TPC Last Forever?
Probably of academic interest
Questions arose as per the liability of the detector itself i.e., aging issues (including shorts and side effects) were raised along with increasing concerns related to grid leak handling. Alexei Lebedev proposed a serie of hardware modification in May 2005 to account for those issues (see What we can do with TPC while FEE are in upgrade attachement).
Relevant to possible software and hardware solutions for the grid leak are GridLeak Simulations of the fields and particle paths in the region near the inner/outer TPC sector gap.
Extensive analysis are also available from the pages You do not have access to view this node and especially (for AuAu) this page QA: High Luminosity and the Future.
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