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UCLA IEP/RHI Group (Huan Z. Huang, G. Igo, S.Trentalange, O.Tsai) R&D for SciFi calorimeters

UCLA IEP/RHI Group (Huan Z. Huang, G. Igo, S.Trentalange, O.Tsai) R&D for SciFi calorimeters STAR forward upgrades. Transformation STAR->eSTAR. Dedicated EIC detector. New, simple, cost effective, flexible technique to build compact sampling calorimeters.

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UCLA IEP/RHI Group (Huan Z. Huang, G. Igo, S.Trentalange, O.Tsai) R&D for SciFi calorimeters

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  1. UCLA IEP/RHI Group (Huan Z. Huang, G. Igo, S.Trentalange, O.Tsai) R&D for SciFi calorimeters STAR forward upgrades. Transformation STAR->eSTAR. Dedicated EIC detector. New, simple, cost effective, flexible technique to build compact sampling calorimeters. Need to be proven. Need for a test run.

  2. Example. Possible evolution of calorimeters in STAR. Forward direction (West side). Should consider: Available space Magnetic Field Radiation Installation/Integration

  3. INTERACTION POINT (June 20,2003) “Cooperative Spirit of SLAC Pays Off for UCLA Researchers.” Test Run T466. In 2003 we tested small EMC prototype at SLAC. We refined construction technique in 2004, and was scheduled for a test run at SLAC in the fall of 2004. Unfortunately after test run was postponed we were not able to continue R&D in this direction at that time. This method of building ScFi calorimeters has yet to be prooven! SLAC Test Beam Facility is very important for calorimetry R&Ds!

  4. As a proof of principle we want to build 4 x 4 EMC prototype using new technique we call it “spacardeon”. If funds will be available we will try to Investigate possibility of building SPACAL type Hcal using W powder/ScFI.

  5. Parameters required for Beam Tests To the presenter at the ESTB 2011 Workshop: please, fill in the table (at best) with the important parameters needed for your tests

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