1. SHMS Heavy Gas Čerenkov Hall C User’s Summer Workshop, August 5, 2008. Garth Huber

2. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 2 Introduction At higher momenta, hadron species cannot be reliably distinguished by time of flight over the 2.2 m SHMS detector stack baseline. At higher momenta, hadron species cannot be reliably distinguished by time of flight over the 2.2 m SHMS detector stack baseline. Good PID can be obtained with a series of Čerenkov detectors: Good PID can be obtained with a series of Čerenkov detectors: e -/ π -  Noble Gas Čerenkov (n-1 < 10 -4 ) e -/ π -  Noble Gas Čerenkov (n-1 < 10 -4 ) π + /K +  Heavy Gas Čerenkov(n-1 ≤ 10 -3 ) π + /K +  Heavy Gas Čerenkov(n-1 ≤ 10 -3 ) K + /p  Aerogel Čerenkov(n-1 ≤ 0.03) K + /p  Aerogel Čerenkov(n-1 ≤ 0.03) Heavy Gas Čerenkov will be the primary means for π + /K + separation above 3.4 GeV/c. Heavy Gas Čerenkov will be the primary means for π + /K + separation above 3.4 GeV/c. 1 m long cylinder with 1.6 m diameter, to be operated at sub-atmospheric pressure. 1 m long cylinder with 1.6 m diameter, to be operated at sub-atmospheric pressure.

3. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 3 Gas recirculation and purification system needed since gas pressure will be changed at higher SHMS momenta. Gas recirculation and purification system needed since gas pressure will be changed at higher SHMS momenta. Maintain sub-atmosphere (0.95 atm) pressure below 7.3 GeV/c. Maintain sub-atmosphere (0.95 atm) pressure below 7.3 GeV/c. Above 7.3 GeV/c, reduce gas pressure to maintain good π/K separation. Above 7.3 GeV/c, reduce gas pressure to maintain good π/K separation. Gap between the `set’ and `K’ curves takes into account the SHMS momentum bite and a possible 0.1 atm error in the setting of the gas pressure regulator.

4. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 4 Focal Plane Coverage Non-magnetic stainless steel pressure vessel. Non-magnetic stainless steel pressure vessel. 1.6m diameter cylinder. 1.6m diameter cylinder. Titanium entrance and exit windows. Titanium entrance and exit windows.

5. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 5 Optical Ray Tracing Studies Co-ordinating design with Donal Day. Co-ordinating design with Donal Day. Four thin glass spherical mirrors (50cmx55cm, radius=175cm) each viewed by a 5” PMT. Four thin glass spherical mirrors (50cmx55cm, radius=175cm) each viewed by a 5” PMT. Asymmetric SHMS envelope dictates different mirror and PMT placements for ±δ. Asymmetric SHMS envelope dictates different mirror and PMT placements for ±δ.

6. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 6 Projected #p.e. assuming 0.6m effective radiator path length and possibleopticalmisalignment. Projected Performance Useful (7 p.e.) lower momentum limit estimated to be 3.4 GeV/c.

7. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 7 Updated Timeline Design:2008-2010. Design:2008-2010. GuideIt studies (CERN optics package). GuideIt studies (CERN optics package). Mechanical design. Mechanical design. NSERC grant application:Fall 2009. NSERC grant application:Fall 2009. New date dictated by DOE timeline and recent comments by NSERC re. possible GlueX BCAL support. New date dictated by DOE timeline and recent comments by NSERC re. possible GlueX BCAL support. Construction:2011-2012. Construction:2011-2012. Delivery to JLab: Winter, 2013. Delivery to JLab: Winter, 2013. Installation in Hall C: Summer, 2013. Installation in Hall C: Summer, 2013. Detector checkout (no beam):Winter, 2014. Detector checkout (no beam):Winter, 2014.

8. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 8

9. 9 Radiator Gas Update The heavy gas originally intended for this detector was C 4 F 10. The heavy gas originally intended for this detector was C 4 F 10. 3M stopped production of this gas some years ago, although it might still be available from a U.K. supplier (>$300/kg). 3M stopped production of this gas some years ago, although it might still be available from a U.K. supplier (>$300/kg). C 4 F 8 O appears to be the optimal substitute. C 4 F 8 O appears to be the optimal substitute. Widely used in the semiconductor industry for plasma etching. Widely used in the semiconductor industry for plasma etching. Easily available from many commercial suppliers. Easily available from many commercial suppliers. Extensively studied by the BTeV collaboration for use in their RICH detector, including beam tests of their prototype. Extensively studied by the BTeV collaboration for use in their RICH detector, including beam tests of their prototype. T. Skwarnicki, NIM A 553 (2005) 339-344. N. Artuso, et al., NIM A 558 (2006) 373-387.

10. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 10

11. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 11 Properties of C 4 F 8 O (OctaFluoroTetraHydroFuran) Gas phase is about 10 times heavier than air (9.19 g/L at 21 o C). Gas phase is about 10 times heavier than air (9.19 g/L at 21 o C). Boiling point: -5 o C. Boiling point: -5 o C. Vapor pressure: 1.7 atm @ 21 o C. Vapor pressure: 1.7 atm @ 21 o C. Stable, non-toxic, non-explosive, non-reactive (except with alkali halide metals). Stable, non-toxic, non-explosive, non-reactive (except with alkali halide metals). BTeV performed 10 year equivalent exposure tests with a variety of materials (plastics, mirror material, epoxies, composites, water). BTeV performed 10 year equivalent exposure tests with a variety of materials (plastics, mirror material, epoxies, composites, water). “No measurable changes seen.” Can pick-up and transport oils. Can pick-up and transport oils. need to avoid contact with organic materials. need to avoid contact with organic materials. Unlike C 4 F 10, it does not destroy ozone. Unlike C 4 F 10, it does not destroy ozone. Rated as having high global warming potential due to its long atmospheric lifetime if released. Rated as having high global warming potential due to its long atmospheric lifetime if released. About $100/kg. About $100/kg.

12. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 12

13. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 13 Schematic Design Non-magnetic stainless steel pressure vessel. Non-magnetic stainless steel pressure vessel. 1.6m diameter cylinder. 1.6m diameter cylinder. Titanium entrance and exit windows. Titanium entrance and exit windows. Four high quality thin glass spherical mirrors (50cmx55cm) Four high quality thin glass spherical mirrors (50cmx55cm) Structurally reinforced outside beam envelope. Structurally reinforced outside beam envelope. A gas recirculation and purification system is needed since the gas pressure will be changed frequently for p SHMS >7.4 GeV/c. A gas recirculation and purification system is needed since the gas pressure will be changed frequently for p SHMS >7.4 GeV/c.

14. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 14 Primary Design Components Protected mirror coatings. Protected mirror coatings. Reference Al coating from Lambda/Ten Optics. Reference Al coating from Lambda/Ten Optics. >90% reflectivity down to 200 nm. >90% reflectivity down to 200 nm. PMTs view enclosure through 1cm UV-grade window. PMTs view enclosure through 1cm UV-grade window. Allows for better isolation of the pressurized cavity. Allows for better isolation of the pressurized cavity. Photonis flat-face 5” PMTs mounted flush to window. Photonis flat-face 5” PMTs mounted flush to window. Bases to incorporate voltage boost between photocathode and first dynode to provide optimum focusing of photoelectrons. Bases to incorporate voltage boost between photocathode and first dynode to provide optimum focusing of photoelectrons.

15. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 15 Integration Will deliver: Will deliver: Pressure tested Čerenkov enclosure. Pressure tested Čerenkov enclosure. Mounted and aligned mirrors. Mounted and aligned mirrors. PMTs with custom bases. PMTs with custom bases. Will need to co-ordinate with JLab staff: Will need to co-ordinate with JLab staff: Location of mounting and alignment fixtures. Location of mounting and alignment fixtures. Design, location and fabrication of gas recovery and purification system. Design, location and fabrication of gas recovery and purification system. Expecting JLab to provide: Expecting JLab to provide: Readout electronics, HV channels, cables. Readout electronics, HV channels, cables. Mounting and alignment on SHMS detector frame. Mounting and alignment on SHMS detector frame. User interface for remote pressure change when User interface for remote pressure change when p SHMS changes. Coordination with U.Virginia (Noble Gas Čerenkov): Coordination with U.Virginia (Noble Gas Čerenkov): Design, and procurement, where appropriate. Design, and procurement, where appropriate.

16. Dr. Garth Huber, Dept. of Physics, Univ. of Regina, Regina, SK S4S0A2, Canada. 16 Funding Cost estimate: Cost estimate: $142k (FY07), Contingency $33k (23%). I intend to submit a Research Tools and Instrumentation (RTI) request to NSERC in Fall, 2008. I intend to submit a Research Tools and Instrumentation (RTI) request to NSERC in Fall, 2008. Timing of request is dictated by necessity of CD-3 granting prior to Canadian funding deliberations in early 2009. Timing of request is dictated by necessity of CD-3 granting prior to Canadian funding deliberations in early 2009. NSERC grants are announced April 1 each year. NSERC grants are announced April 1 each year. If the NSERC grant request is successful, it will count as a foreign contribution to the Hall C upgrade and help relieve pressure on the 12 GeV cost book. If the NSERC grant request is successful, it will count as a foreign contribution to the Hall C upgrade and help relieve pressure on the 12 GeV cost book.