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Title: Compare 100 GeV/n Au Run 2010 with Run 2007

Technical Report ·
DOI:https://doi.org/10.2172/1007885· OSTI ID:1007885

With the very successful commissioning of the vertical stochastic cooling in 100 GeV/n Au Run 2010, the IBS (intra-beam scattering) is no longer the dominant factor in terms of the integrated luminosity. A new luminosity model is needed, where the beam intensity lifetime is more important and the burn-off needs to be accounted for. Toward this goal, a brief review of the Run 2010, compared with Run 2007, is presented.

Research Organization:
Brookhaven National Lab. (BNL), Upton, NY (United States). Relativistic Heavy Ion Collider (RHIC)
Sponsoring Organization:
DOE - Office Of Science
DOE Contract Number:
DE-AC02-98CH10886
OSTI ID:
1007885
Report Number(s):
BNL-94622-2011-IR; R&D Project: KBCH139; 18031; KB0202011; TRN: US1101795
Country of Publication:
United States
Language:
English

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