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The Mechanical Integration Challenge for New Tracking Detectors in STAR Jim Thomas 07/10/2006

The Mechanical Integration Challenge for New Tracking Detectors in STAR Jim Thomas 07/10/2006. The Challenge . Design, build and install the HFT on the East end Keep the SSD (which is supported from East and West Ends) Design, build and install a new IST from the West end (?)

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The Mechanical Integration Challenge for New Tracking Detectors in STAR Jim Thomas 07/10/2006

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  1. The Mechanical Integration Challenge for New Tracking Detectors in STAR Jim Thomas 07/10/2006

  2. The Challenge • Design, build and install the HFT on the East end • Keep the SSD (which is supported from East and West Ends) • Design, build and install a new IST from the West end (?) • Keep these detectors thin; ~1% per layer • Keep the region of 1 to 2 units of rapidity clean and low mass • Add new forward tracking detectors

  3. The SSD is a Beautiful Detector • The SSD is thin • 1% - double sided Si • The SSD lies at an ideal radius • 23 cm - midway between IP and IFC • The SSD has excellent resolution • (rumor says better than design) • The SSD is too large to be replaced • The money is better spent, elsewhere

  4. Existing IFC Volume At left is cone provided by SUBATECH. The lower left photo shows the cone with SVT/SSD utility runs under outer shell. The lower right photo shows the cone with vacuum beam pipe installed. The beam pipe is trapped in the cone by its flanges and the internal pipe supports bellow. Ralph Brown

  5. Existing IFC Volume The left photo shows the SVT mounted on the support cone with SSD support rings. You must remove the SVT to get at vacuum pipe supports. The right photo shows the SSD mounted on the cone between aluminum support rings. You must remove the SSD to get at the SVT. Ralph Brown

  6. SVT Detail – beam pipe size & mounting issues … Note Double Cone

  7. IFC Volume Options • Remove existing Cone, SVT, SSD, and Beam pipe as a complete unit for future heavy ion running (low risk of damage). Replace it with a new similar cone structure with SSD support plus utilities and new beam pipe. Requires fabrication of a new Beryllium/Aluminum pipe, low Z cone structure, and duplicate SSD utilities/mount (lots of time and money). Include HFT mounting interface and add to project proposal (plus Photon Converter?). Ralph Brown

  8. Existing IFC Volume Cross-section view of the existing STAR IFC west volume includes: Be/Al Beam Pipe, SVT, SSD, Cone, SVT/SSD Utilities (cables/hose) and RDO Boxes, FTPC, IFC Air Manifolds. You must remove the cone with SSD/SVT/Beam-pipe as a complete unit with the STAR Detector in the Assembly Building. Ralph Brown

  9. Review of the Challenges The challenge for the East end: • The East end must support the HFT, SSD, and all utilities • Challenging, but can take advantage of the existing cone The challenge for the West end: • Support the SSD and its associated utilities and cables • with a new double layer cone • Stay out of the 1-2 units of rapidity interval (this is difficult) • Probably requires putting utilities close to the beam pipe • Preserve the HV integrity of the IFC • Use a graded cone shield at HV, if necessary. Probably cannot go closer to the IFC than done by the existing cone.

  10. IFC Volume Options • Remove the SVT and its utilities from the cone structure along with RDO boxes and reinstall existing beam pipe and cone with SSD and its utilities (SVT never to return). Low cost and can be done in one summer shutdown. Ralph Brown

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